SCIENTIFIC ABSTRACT VORONTSOV-VELYAMINOV, B.A. - VORONTSOV-VELYAMINOV, N.P.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R001861010010-3
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: November 2, 2016
• Document Release Date: March 14, 2001
• Sequence Number: 10
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

of the Uaiverse WV/3717
Ch. 2. Dwarf Pin-.,Mv-s 85
Plana' hunters 85
5,1!%massim, of discoveries 88
Thn clprfper 3mto the forest., the thicker the voods 93
Oux neamst neigbbors 99
Jauxnt-.y to Hermos and sojourn on Hermes 105
Ch. 3. Visible Nothingaess 113
Earbingers, of dcom [comets) 113
Celestial zbAmelaecas 120
Ral.ley's discovery 128
Short-period comts 132
Family ne-mbers and strangers 136
Pips,xlvvery of c--mets 140
1"s of Comets 143
711-~- vi F;;M-le nothingness 147
Oau--a of I=ineseence of comets and their chemical compositiorL 151
Rasser. for the fermation. of comet tails 154
Eae.-W)s --ollision, with a comet 157
"-Aln of COMAS 16o
c5xd 3/8

Fe!afnar!~s of tha Universe
ch. 4. 13hc&.!mg Stars and Star Shawers
Shcrct.ing stars and otovas from the sky
ImAge and Identification of meteors
St---- shwers and meteor istrews
More dnr-,ailz- on meteors
mftteors
of mateoro
F)U.MU&n-t8 Of CrDMAS
M.n,t-a%r.q J,n the atmosphere
Ch. 5. CAlestial Stones and Dust
strcmes (mete-orites]
and age of meteorites
Ch~--EUt.:al c,:.qposition of the earth and meteorites
for parents
-i"awm,
01,.b:~.,r =.Atorv of meteorites
5ingusakil me-becirite
mett6rite
0:~ls-stial bowardmetnts
light and earth's gaseous tail
6e=,-Al5 =&"Zftes
l7ard 4/8
SW/3717
163
163
168
171
175
184
18T
192
199
23-1
217
222
228
232
235
240
245
250
255
26o
*3

reatures of the Universe
Bright and dark nebulae
Interstellar dust
PART n. M GkMM VORM
SM/3717
281
Ch. 6. 2M Sun., Our Nearest Star 291
First 80quaintance, 291
Mae sphere of light 294
Rven the sun in not spotless 298
Observation of the invisible and the anatooW of the sun 301
2he mantles of the sun S06
World's highest fountains 36�
tordto corona, and its r1steries 311
How three astronomers cheated nature 315
Bunts chemistry 319
Story of tva strangers 320
Ch* 7~ Stars.4 the Distant Suns 327
Understanding the Incomprehensible 327
Timinogity of sta~z 328
Spectraj, the passports of stars 330
Card 5/8

Features af the Universe
SOOTIT
What is the composition of stars and %ft do they have different passports? 334
Thermometers for stars 336
Spectra as indicators of the distance of stars 337
Plumb line in the unfathomed reaches of the universe 339
Motion of immobile stars 343
Regulation of star notion 345
Where are ve being carried? 347
Measuring the stars 349
Binary stars 350
Devil's stars 357
Cephelds, the pendulums of the universe 359
Physically variable stars 361
Portrait gallery of colored stars 363
Portraits of white stars and the history of their drawing 368
Anatomy of the stella atmosphere 3T4
In the neighborhood of the sun 377
Bu's neighbors 379
Distribution of the luminosity of stars 3M
Reccirding the stars on the luminosity diagrom 388
Card 616

Features of the Universe
Ch, 8. The Islands of the Universe
Mileposts and the structure of the universe
Dispersed and spherical constellations
Islands of the iiaiverse
Interaction of galaxies
Infini,V and our address in It
From the nucleus of an atom to the metagalwW
Ch. 9. The Life of Stars
Haw old are stare and the Milky Way?
What feeds the stars?
1ftc1ei and nuclear reactions
wFeeding cycle* of stars
Internal structure of stars
Ch. 10. Self-Destroylbig: Stars
Spinning stars
Inflated atmospheres
Stars vhich give off gas
Stars Vhich tbrow off their mantles
From superstar to enigma
Card 7/8
SOV/3717
391
391
399
404
412
416
420
423
423
428
430
440
449
449
450
453
457
466

Features of the Universe SOV/3717
Ch. 3-1. Universe of Dispersed Gases 474
Clarification of nebulae 474
Diffuse nebulae
Planeta~y nebulae .479
Nebular gas 481
luminescence and the nature of nebulae 483
Interstellar gas 485
Ch. 12. Radio Contact vith Space 493
Radio echo in astronomy 493
Solar radio emission 498
Cosmic radio emission 499
Ch. 13. Genesis of Worlds 503
Cosmogony according to TAplace 503
Jeanst hyporthesis and Its collapse 5o6
Theory of Academician O.Yu. Shmidt 509
Studies of Academician V.G. Fesenkov 518
Origin of the diffuse nebulae., interstellar medium, and stars 521
AVAIIMIZ: Library of Congress (QP981.V84)
JA/mh
Card 8/8 6-21-6o

VORONTSOV-VELOYAMIBDV, B.A.
-.- I - 1:~,- ,-
A now type of celestial bodies. Astron.teir. n0.202:8-10
J8 159. (MIRA 13:4)
1. Gowudarstvennyy astronomichoskiy institut im. P.K.Shternberga,
Moskva.
(Galaxies)

FRANK-KAKMINTSKIY, D.A.. prof., otv.red,; YOROUTSOV-VELITAKINOV, B.A,,
red.; SHORODINSKIT, Ta.A., prof.,
starshiy nauchnyy sotrudnik, red,; SAG13131, R.Z., uladshiy
nauchnyy aotrudnik, red.; SAMSO]MMO, L.V., red.izd-va;
SWCHAIKO, G.N., takhn.red.
(Transactions of the sixth conference on cosmogony; extra-galactic
astronomy and cosmology] Trudy shestogo soveshchaniia po vopro-
sam kosmogonil, 3-7 iiunia 1957 g.; vnegalBktichasksia astronomiia
i koemologiia. Moskva, 12d-vo Akad.nauk SSSR, 1959. 273 p.
(MIRA 12:12)
1. Soveshchaniya po voprosam koemogonii, 6yh, 1957. 2. Chlen-
korrespondent Akademil pedagogichaskikh nauk SSSR (for Vorontsov-
Vellyaminov).
(Cosmology--Gongreases)

VOROUTSOV-VEL'YAKINOV, Boris Alsksandrovich
(Atlas and catalog of interacting galaxies] Atlas i katalog
vzaimodaistvuiushchikh galaktik. Moskva, Gos.astronomicheskii
in-t im. P.K.Shternbarg pri Mosk.goo.univ. Vol,l., 1959.
(KIRA 13t4)
(Galaxies)

PEREL12 YU.G.; POPOVs P.I.; MARMOV, D.Ya.; KUNITSKIY, R.V.;
BAUM, V.V.; KULIMY, K.A.;
SHISTOVSKIY, K.N.; TSVETOV, R.I.; BRONSHTE1,11, V.A.; DAGAMp M.H.;
MOGILKO, A.D.; SEMAKIN, N.K.; WITRIYEN, L.S.; IZOTOV, A.A.
Mihail Evgenlevich Nabokdv; obituray. Buil.VAGO no.28:60-62
f6o. (14MA 14:6)
(Nabokov, Mikbail Evgenlevich., 1887-1960

--r
UX,
11 r
1:; v' 3.
I- v
a
i
R
P. V
f laic

85108
2. 71 /e S/033/60/037/004/014/015/XX
E032/E314
AUTHOR: Vorontsov-VeL'Yaminov, B.A.
TITLE: Partial Gas Den--si-fi-es ~inthe Come~ 1942g Whipple
PERIODICAL; Astronomicheskiy zhurnal, 1960, Vol. 37. No. 4.
pp. 709 - 715
TEXTs In a previous paper (Ref. 3), the present author
discussed the photometric structure of the comet 1942gusing
direct photographs obtained at the Abastuman Observatory.,
It was established that, within experimental error, the spatial
photometric densities in the head of the comet are inversely
proportional to the square of the distance from the nucleus
and the brightness seen in projection is inversely proportional
to this distance. The diameter of the coma in the best
photographs could be extended up to 6 x 105 km but this does
not, of course, indicate that the diameter of the comet was,
in fact, infinite. Using Imperial 1200 plates, G. Tevzadze,
working at the Abastuman Observatory obtained four good
photographs of e spectrum of the somet on February 3 and
March l1v 30 and 31, He used an 811 camera with F = 100 cm
and a 1 deg. prism. The dispersion on the spe~;trograms
card 1/~

85108
S/033/60/037/004/014/015/XX
E032/E314
Partial Gas Densities in the Comet 1942g Whipple
0
was 170 A/mm in Hy . The present paper gives an account
of the information obtained from the best spettrogram which
was obtained on March 11 (exposure 2 hours, length of
spectrum about 12 mm). The motion of the comet was slow and
hence its images were undistorted,, Weak traces of the cometary
tail are seen in the photograph at an angle of about 30 0 to the
direction of dispersion. The spectrum of the nucleus can be
clearly seen. Bright emissions in 3883 CN, 4730 C2 and 4050 C 3
are present in the spectrum of the head, The photographic
brightness was measured at 500 points on the spectrum and the
intensity of the centre of the image in the CN radiation (maxi-
mum intensity) was taken as the unit of the intensity. Fig. I
shows the isophots in the spectrum of the comet. The numbers
show the intensities in hundredths of the above unit, The
absolute monochrom tic emission in the above three bands was
found'by reference to stellar spectra. The number of
molecules inside the 0;005 isophot which are responsible for
Card 2/4

85108
S/033/60/037/004/014/015/XX
E032/E314
Partial.Gan Densities in the comet 1942g Whipple
33 32
the above three bands was found to be 1-3 x 10 761 X 10
1031, respecti Ively.(radius of coma 3.7 IL05 km). The
and 2.7 x
total mass of the coma was found to be 7.5 X~.10110 S and Is
10 10 -
mainly due to CN and C. (4.4 x 10 and 2.9 x 10 respectively).
The densities are inversely proportional to the distance from
the'nucleus and are of the order of 1011 molecules near the
nucleus and about 2 molecules of CN, I molecul of C 2 and
0.04 molecules of C 3 per cm3 at a distance of ;-7 x 10 5 RM.
The calculated number of molecules based on the apparent
brightness of the comet and the Zanstra method is in agreement
with accurate spectrophotometric determinations.
Acknowledgments are expressed to Professor Ye.K. Kharadze
of the AbastumAni Observatory for supplying the spectrograms.
Card 3/4

85108
S/033/60/037/004/014/015/XX
E032/E314
Partial Gas Densities in the Comet 1942g Whipple
There are 4 figures and 10 references: 4 English, 1 German
and 6 Soviet.
ASSOCIATION: Gos. astronomicheskiy in-t im. P.K. Shternberga
(State Astronomical Institute Imeni
P.K. Shternberg)
SUBMITTED: April 8. 1960
Card 4/4

VORONTSDV-VZLIYAMINOV B.A.
1!
Variations In the spectrum of the planetary nebula IC 4997 ard
their origin. Astron.zhur. 37 no.6:994-1000 N-D 160. (YIRA 3,3:12)
1. GogudarstvenMy aatronomicheakiy institut im. Me Shternberga.
(Nebulae-Spectra)

voRoNTsov_VIIL,YM3OV, B.A.
Is 37 no.6MI22 3~-])
Classifying line spectra of stars. Astron-zhur
160. OaRA 13s12)
1. GeoudarstvanMy astronomicheakiy institut im. P.I.Shternberga.
(Stars-Spectra)

VORON"q-VXL'YAMINOV, B.A.
Ring galaxies. Astron.zhur. 37 no.3:381-386 My-Je 160,
(MIRA 1316)
1. Hookovskiy gorodskoy pedagogicheskiy institut Iment V.P,
Potemkin&. (Galaxi es)
-1

VORONTS&-VELIYAMII-OV,- B.A.; SAVELIMVAp M.V.
SpootrophotometrY of a aupernoVa in UGG "96. Astron.tair. no.2.16:
2.3 D 160* OaRA 14:4)
1..GosudarstvennYY astronomicheskiy inatitut im. P.K.S hternberga.
(stars, New)

ARKHIPOVAI V.P.; IMUCHAYEVA9 O.D.; VORONTSOV-VELIYAMINOV, B.A.
Spectrophotometi-j of AG Pegasi. Astron.tsir. no.223:17-18 Jl
161. (KIRA 15:3)
1. Gosudarstvennyy astronomicheskiy institut im. Shternberga.
(Stars, Variable--Spectra)

_q/0 /61/000/002/004/016
,-35
AOO11AOO1
Translation from: Referativnyy zhurnal, Astronomiya I Geodeziya, 1961, No. 2,
p. 21, # 2A222
AUTHOR: Vorontsov-Vel'yaminov, B.A.
TITIEs Visible Residues of Three More Supernovae
PERIODICAL; "Astron. tsirkulyar", 1960, mava 5, No. 211, pp. 25 - 27
TECT: The author-describes three nebulae from the Abell list, identified
by him with Supernovae. The nebulae were studied on the charts of the-Palomar at-
las. Nebula Medusa (7h23M.5, +21~027'; 1900). A large filamentous formation in
the shape of the crescent having the size 8' x 61. Filaments complementing the
nebula to a full ellipse are on the verge of visibility. The appearance and
brightness of the nebula in red and blue rays are almost Identical; consequently,
nebulium green lines are bright in its spectrum in addition to Hw . This indicates
considerable ionization and excitation. According to its coordinates the nebula
is identified with radio source 2C - 653 from the catalogue of Shakeshaft, Rhyle
et al. and Supernovae of years 829 and 1430 AD. Nebula Crescent (1h 24T2, +57050',-
1900) has exactly the same filamentous structure as Medusa but weaker. In blue
Card 1/2

.9/035/61/000/002/004/016
Visible Residues of Three More Supernovae A001/A001
rays Crescent is considerably less luminous than in red ones. The nebula is close
to two Supernovae of 722 and 902 AD and probably is a residue of Supernova 902 AD.
b
Nebula Semi-ellipse (2.3 54mi, + 61054'1 1900) represents an are of ellipse con-
sisting of thin and weak filaments traced approximately by 2100 and only I (?) wide.
The major axis of the nebula amounts to 311. The brightest are part is slightly
visible in blue rays, consequently, emission in lines N, and N2 Is considerable.
Several Supernovae are located close to the nebula. The most probable is the iden-
tity of nebula Semi-ellipse with Supernova 3692. There are 6 references.
N. Perova
Translator's note: This is the full translation of the original Russian abstract.
Card 2/2

BAZYXIK, V.V.; BRONSE V.A.; LORONTSOV431LITANNOV, B*A- ; DAGAYSYs M-M-
DMIIRIYEV. L. So IZOTOV, A. To: ~SKBG R. V-
XARTrxovl D.U.; XDrCMOMOV. Te.T&.; HOGILKO, A-Do ; m.~Imj I YU.G.;
Popov, r# ro -, REZWIXOV, L- L ', SVZTLOV, R. I.; SEKAX3, h-Ko;
SHISTOVSKU, I.I. :
Mikhail Evgenlevich Nabokov; obituAry, fiz. Y shkole 20 no-3tllO-
ill My-is 160. (XIRA 13:11)
(Nabokov, Mikhail Ngenlevich, 1887-1960)

VORONTSOV-VELOYAMINOV, B.A., doktor fiziko-matematicheskikh nauk
I Congress of astronons in California. Nauka i zhiznl 28
no.12:14-20 D 161. (MIRA 15:2)
(Astronomy--Congresses)

vu~ c: ",61
os:
%t ti..

Doo rilA., n ~C llilr.)~-txli
`2 'Ta
no. 1:7
st -or.
1. Gol-vd,rztv;IT.~y

VORONTSOV-VELIWIII-IOV, B.A., prof. (Moskvu)
.Interaction be*een gala~les. Fiz. v shkole 21 no.1:11-14
ja,v 161. (MIRA 14:9)
1. Chlon-korrospondent Akademii podagogichooklkh nauk MrSR.
(Galaxies) I
0

VOROL'TSOV-VELOYAMINOV, B.A. . I
Pavel Petrovich Parenago (10,06-1960). Ist.-astron.iosl.
no.7:335-394 161. 1 (MIRA 14:9)
(Parenagos Pavel Petrovichp 1906-1960)
I

VORONTSOV.;%rZ,L',YAMINOV, B.A.
-I
New planetary and peculiar gas nebulae. Astron.zhur. 38
no.2:375-376 Mr-Ap 161, (MIRA 14:4)
1# Gosudarstvennyy astronomicheakiy institut Im. P. K.
Shternberga.
(Iqebulas)

10
VOROMOV-VEL'IYAMINOV, B.A.
Changes in the spectrum of the planetary nebula NGC 6905. Astron.
zhur. 38 no.2:247-249 Mr-Ap 161. (KLU 14.4)
1. Gosudaretvennyy astronomieheakiky institut im. P. K. Shternberga.
(Nebulae-Spectra)

j VWNDGORSKAYA, Aliza
J& la
-A -Imandroviph
yqROX250V.~' ~NOVt BU
Arkadlyevna; Frinimall uchoLsti7es TS-ITSIN,, F.A.; FONOMAREVAq
G*A.j MAIAROV,, A.N.; ZUKARMN,, B.V., prof., otv.red.;
YEMUKOV, M*S., tekhn.red.
(Morphological catalog of galaxies, Part 1, Catalog of 7,200
galaxies vith declinations from 90 to 451 Morfologichookii
katalog galaktik. Chast' 1. Katalog 7200 galaktik ot
90 do 45 sklonenita. Moskva, Izd-vo Mook.univv., 1962.
205 p. (Moscow. Universitet, Gosudarstvennyi astronomiches W
institut. Trudy, vol.32). (MIRA 16s2)
(Galaxies-Catalogs)

VORONTSCV-VELIYAMOVp BeAs
fttragalactic astronomy and cogmgony at conference in C"Ornia
.in 1961. Astron.zhur. 39 no.U174-181 Ja.F 162o
(KERA 1512)
(Astronomy-zongresses)

ASUPOVICIIII.S.; BAKUL11-1P.I.; VAYITAZV,AJ-I.; IRONSIITEfI,V.A.; 1311GOS)LAVSKAYA,
N.Yaddeceasod)l VASILfYSV.,O.B,.; GRISHINjN,I.j,DAGAYEVj*-HJ1.j
DUR-WGf=,K.K-Ldeceased]; WULA-'.OV,G.P.; ZO!!nI,I.T.;
OII'OV,Ye.L,; OLIKINSKIY,P.G.; M-6ITSKI7,R-.V.;
ORLCV,S.V.Cdeceasod]; POPOVIP.I.; FUSHKOV, N.V.;
RYBAKOV, A.I.; HYADOV,Yu.A.; SYTITISKAYA, N.V.; TSESEVICII, V.P.;
SUCHIGOLEViB.M.; VORONTSOV-VLIL 'YAM1IOV,B.A.j red.; F(jIUFAI,2VA,G.A.,
red.; KRYUCHKOVA,TIr--.-UM---r0-ff--
(Astronomical calonder; permanent part] Astrononicheskii kalendar';
postoiannaia chast'. Izd.5., polnootliu perer. Otv. red. P.I.Balculin.
Red.kol.V.A.Bronshten i dr. Moskva, Gos.izd-vo fiziko-matem.lit-ry,
1962. 771 p. WIRI 15:4)
(Astronomy-Yearbodks)

JQRONT~01~nYLL~YA!9XQV-,-B.A.
Some aspects of the Ambartsumian hypothesis on the origin of
galaxies. Vop.kosm. 8s27-31 162. (MIRA 15:7)
(Galaxies) (Coamogonv)

AGEXYAN, T.A;; VORONTSOV-VELYAMIN B.Acj GORBATSKIY; V.G.; DRYCH,
d07 'V -- OV I - SOBOIZV, V.V.; MIKWLDV, A.A.,
A.N* , A.; MELINIKOV, O.A.P
otv. red.; KULIKOV, G.S.,, red.; AKMIROD, I.Sh... tekko. red.
[Course on astropbyBics and stellar astrononVIKurs astrofiziki i
zv,eadnoi astronomii. 2. izd. Moskva, Fiznatgiz, Vol*2 'T.A.
Agekian i dr. 1962. 688 p, WRA 16':11
(Astropbysice) (Stars) (Nebulae)

VORONTSOV-VEL'YAMINOV, Boris-Aleksandrovich., prof.; KULIKOV, G.S.,
red.; BRUDNO, K.F.,--%b~-
(Collection of problems and exercises in astronomy] Sbornik
sadach i uprashnonii po astrqnomii. Izd.5- Moskva, Fizmat-
giz, 1963. 279 p. 04TRA 160)
(Astronomy-Problems, excerctseij etc.)

YORONTSCV-VEL'YAMINOV9 B. A.
Dark matter in galaxies. Astron. zhur. 40 no.1:85-93 J-F 163.
.(Mjn 16: 1)
1. Gosudarstvennyy astronmicheiskiy institut im. P. K.
Shternberga.
(Galaxies)

VORMTSOV-VELLUM011) B. [Vorortoov-Vellyaminov,, B.]t prof.
Vhat will aatronauts find on t1he mcc-n? Nauka i tekh m:Ladezh
15 no.6t7-9 Je163.
1. Moskovski durzhavan universitet,

VORONT !Y&INOV,,-Boris Aleksandrovich., prof.1 FAYNBOYM, I.B.,
.
red.; RAKIT.U4, I.T.,, tekhn. red.
[Galactic spaces) Prosttory galaktik. Moskva# Izd-vo
"Znanie," 1963. 47 p. (Novoe v zhizni., nauko., tekhniko.
IX Seriia: Fizika i khimliav no.23) (MIRA 17:2)
/I

5/033/63/040/001/010/016
E032/9514
AUTHOR i Vorontsov-Vellyaminov# B_
TITLE: Dark matter in galaxies
VERIODICAL: Astronomicheakiy zhurnal, v.400 no.l. 1963, 83-93
TEXT: This is a review paper concerneil with the diStribution
of dark matter of all types and based on a.study of a lak-ge-
number of direct photographs taken mainly from the Hubble Atlas
of Galaxies compiled by A. Sanda~e (1961). -Thq.,subject matter
is considered under the following headingst 1)II-i'lliptical galaxies,
2) lenticular galaxies, 3) spiral galaxies. 4) particularly,
noteworthy cases. and 5) dust in the nuclei of spirals.
Conclitsions: It is shown that the dynamics-of diffuso.matter in
galaxies is much more complicated thAn is, usually. assumeds It is'
estimated that the thickness of the layer of dust.in many galaxies
seen edgewise is often-greater than in-Pur galaxy and reaches up
to 1000 Pa. There is 1 table.
ASSOCIATION: Gos. astronomicheskiy in-t im.'P. K. Shternbergd
(State Astronomical Institute imeni P,K,Shternberg)
SUDMITTED: January 29, 1962
Card I/J

VORONTSOV-VELOYAMINOV, Boris AleksapArovich,- KULIKOV, G.S., red.
(Essays on the universe] Gellerki o Vselennoi. Izd.5., dop.
fl,oskva, Izd-vo ffflauka," 1964. 552 p. (MIRA NO)

VORONTSOV-VEL'YAMINOV, B.A.; KOSTYAKOVA, Ye.B.; DOKUCIIAYEVA, O.D.;
ARKHIPOVA, V.P.
Absolute intensities of emission lines of planetary nebulae. Part 1.
Astron.zhur. 41 no.2:255-263 Mr-Ap 164. (MIRA 17:4)
1. Gosudarstvennyj astronomicheskiy institut im. P.K.Shternberga.

VO.ROttfS()V-kFEL",-'f~MIN,')V, B.A.
Slimllrarit,z of JIGC 5195 and 3077 with the eiplod-Irg galexy
Y82. Astron. tsir. no.266:1 0163. KRA 117:5':
1. Gosudars*.Vennyy asti-cnomicheakly institut irmini Shternba-rga.

VOROjUSOV_VF,LyA~jINOV) B. A.
t'r eJ r
na in the structure of galaxies and n I
"Evidenee of magnetic-like pheno!W
cosmological meeting."
report presented at the Intl Conf on CoSmolog~j Padua, Italy, 14-16 sep 64.

ACCESSION NR: AT4038537 8/2623/62/000/118/0003/0035
-PTHO14 Vorontosov-Vellyaminov, B. A.
TITLE: A now catalogue of planetary nebulae
gQURCE. Moscow. Univ. Goa. astron. Inst. Soobshch., no. 118, 1962, 3-35
'TOPIC TAGS; astronomy, astrophj~sics. nebula, planetary nebula
L
A13STRACT: This catalogue of planetary nebulae contains not only the accepted planetary
-nebulae, but also possible objects of this class listed by Haro and Perek; the total listing
1& 591 nebulae. The first column In the catalogue gives the assigned number; the second
column -- the NGC, IC number or other source, abbreviated as described In the Russian
text. Possible planetary nebulae are denoted by an accent mark. Coordinates are for the
epoch 1900. 0. The table gives the type according to the author's former classification and
dimensions W seconds of are (if not marked with a minute sign). D In the table means that
the disk was visible. The upper limit of 10" to given on the basis of spectroscopic obser-
vations made by Moscow observers; m. is the Integrated photographic magnitude; RE is
the relative exposure (Curtis); H Is the author's valuo of the average surface brightness
in magnitudes per square minute of arc. Roman numerals are used to denote the surface
brightness frora the Palomar Sky Atlas on the scale: I -- very bright, M -- very faint,
Card 1/2

ACCESSION NR: A 38537
0 -- Invisible. Sp denotes the spectral classiffication of the nebula on the scale: Ilow
excitation (N1 and ~~ faint), M -- high excitation (-A 4686 Hell strong). The excitation
was estimated from absolute spectropbotometric data (or relative data when in brackets).
For other nebulae tlia observed lines are noted. Those in brackets refer to the author's
observations; (-) means that no trace of a spectrum could be found; m* and Sp* are the
photographic brightness of the nucleus and its spectrum; V is the radical velocity and &V
the velocity expansion. Values of nuclear temperature and proper motions are given
In the former catalogue In the author's book Gasnebel'und, Neue Sterne, Berlin, 1953.
OrIg. art. has: 1 table.
ASSOCIATION: Gosudarstvenny*y astronomicheskiy Institut Moskovskogo Universiteta
(State Astronomical Institute of Moscow University)
SUBMITTED: 00May61 DATE ACQ: 18Jun64 ENCL: 00
SUB CODE: - AA NO REP SOV: 006 OTHER: 009
:.Card 2/2

VORONTSOV-VELOYAMINOV, B.A*
1-1- 1-11- 1 .. I ~ ~ ~ ~. I- e- , - -
Nuclear regions of -ralaxles. Part 1: Pho'o=et:-'c character-'s"cs.
Notron. zhur, 42 no.6:1168-1183 N-D 165. Ova""I"I 19: 1)
1. Gosudarstv9nnyj astronomicheakiy institut lin. P.K. ShternberCa.

voin.mai-vELlyAmmov, B.A.
Globular clusters in galayies. Astron. zhur. 43 no. 1031-2312
Ja-F 166 (MIRA 1912)
1. Gosudarstvennyy astronomicheskiy Institut imeni P.K. Shtern-
berga. Submitted March 18, 1965.

VORONT-SOV-VFl,'YAMI NOV) B.Aep profo
-----------
Verification of ocami -gical theories b.7 obreniations, Ze=vi vaels
1 no.?-a6,0-63 Mx-Ap IE5. (MIRA 18:8)

IAYPVA, O.n_- ARK111MIA,
Y-,. B.
V, P.
s of F, -,as. Part 2.
Alh~rllllt,e nt--4r:3l' ties of ss, UU,
no*- 730-73") L---Ag 165. (MIRA 18:8)
G-5udarjtvernyy instl tuL im. P.Y.Sh.~A-rnberga.

VORON7SOV-Vk',LIYAMI V.
NO KO"WAKOVA, Yo.b.; MIJOHAYEVA, O.D.1
AYTM-POVA, V.P.
Revined absolute intensitiez; of thn emis-,ion lines of 25 plaratary
nobulae. An-tron.zhur. 42 no.2--464-466 Mr-Ap 165. (MIRA 18:4)
1. Gosudarstvennyy astrouor-Ocheskiy inatitut ir, ?.K,Sh1wernbc-rga.

/VT 1~ VE L-
WO) 6
KULAGIN, S.G.; KOVBASYUK, L.D.; DAGAYET, M.M.; ROZMMLTUM. N.D.; YEGORCHOKO,
I.P.(Irkutak): KAVUIN; A.I. (Irkutsk); KONSTANTINOVA. T.G. (Irkutsk);'
K=INA, V.A. (Irkutsk); KMIN, G.T. (Irkutsk),- SAZONOTI, Z.G.,
(Irkutsk); CHK~Nl , L.I. (Iitutak); CHBRBMH. N.S. (Irkutsk);
DZMIDOBICH, Te.G.'; BRONWEN, T.A.; TMONTOVA, N.S. (Leningrad);
PIROVA, N.B.; DOKUCHATSTA, O.D.; KATASIff, L.A.: XLTAXOTIO, N.A.;
PARINAGO. P.P.; SHCHMMINA-SAMOYWVA, I.S.; KASEVICH,,A.G.;
RTABOT, Tu.A.; SRCFMGLOY, V.P.; PIMI, lu.G.~ MARTINOT, D.Ta.;
FL'MSKIT, V.T.; YORONTSOT-YELITAKINOT, B.4v;_ ZIGM11 FOTU.;
BAKULIN, P.I., otv,red.;,-RA lit. red. AMAMOV, S.N.,
takhn.red.
(Astronomical calendar) Astronomichaskii kalendar'. (A yearbook;
va-kable section for 19591 Exhagodaik.' Peremennsis chast', 1959.
Rad.kellegiia P.I. Bakulin i dre Moskva, Gos.izd-vo f~zika-
matem.lit-ry. 1958. 370 P. (Tsesoiuznoo astronomo-geodazichaskoe
obghchostro, no.62) (MIRA 12:2)
1. Gosudarstvannoye astronome-goodeziah&skoys obehallestva (for Kulagin,
Kovbasyuk, Damidovich). 2. P'loskovskoye 6tdeleniya Veasoyuznogo astre-
nomo-goodesichookogo obahchastva (for Dogayev, RozenblyiT, Bronshten,
Ferova).
(Astronomy~-Tesrbooks)

ACC NR, SOURCE CODE: UR/0384/66/000/003/0006/0008
:AVj'HOR; Vorontsov-Vellyaminov, B. A, (Professor)
iORG: none
TITIX; Puzzling phenomena in the world of the galaxies
SOURCM Zemlya i vselennaya, no, 3, 1966j, 6-8
TOPIC TAM galaxy, galactic structure, gravitation efftet
i
ABSTRACT: The author suggests that it may soon be possible to discover new properties
and laws associated with galactic systems, indicating a change in the mass and gravita
tional fields of these systems with time. Several examples are cited to support this
viewpoint. These concern the extremely high rate of gas flow from the centers of gal-
axies, the discovery of radiogalaxies with their peculiar properties, and certain othe
phenomena which show that the existing forms of stellar systems cannot be explained by
known laws of mechanics. Drawing attention to recent developments in the field of mag
netobydrodynamics, the author states that certain phenomena observed in other galaxies
can apparently be explained as manifestations of magnetic forces.. Orig. art. has: 2
CODE; 03/ 'SUBK DATE: none
C..,d 1/1

ACC NRs v
,IT60275821 U.V(;
Of
MG., nono
TITLE; Naw studios of ral=ios
dy i wolonnaya (Stars and tho wlivoroo)* 1/1%;cov, Izd-vo Znaniya,, lc)66,
SOU11U,; ZVOZ
TOPIC 'TAGS: Calactic structuro, grwditat"Lonp maZ;Iotohydrodyn,Izicz
ABSVIkG7': it, was tmtil rocoatly '%,.Aa'u a sln~,Io of
controllcd tna uorld of -.0 nxioc.
and havo sho,.-n that wo still ov littlo abou-k~. tho fuc~ozn a
clu3tora. 7hoy su,^f,~ast w0 cxO uIcaut to dincovaz, now propoc'.-ios "d row lr-W!l
v.'Ach involvo sy3tcmms havin.- coloso-al massc3 and diotouncoO. -~Irccnt._3y a rnct~ scionco
patodl as ma,,fiotohy~Lrodyna:Aosa it doalr) t`.o =vc ont of ionlz-
dosir
cd grasoa. Tho -prevnca of a maZaetic flcld in our rlalc:y wz~,- pzovocl rOC6-,.-.Iy ':-,;r
direct, obsor~rations. However gc_1a::io3 ~,onsistl oil stars (oftaa vary old) ind tho ma-
n.-atie field ccuinot control the stars 0-nd tharofora cannot t'ho of Z;ala-
Voro aro gala~do3 in whicla one lb_-anch =:1s ri~~it zaid ,ho othoz lof.;
vlnycios (spiral and alliptic) ara 1mova to be joincd by a bziciza
LIC-OrA--112

ACC NRi A-6027582
d-4 s t an c oa of -'OjrCL-Cds of thou.-1--nar, 01. li" y0a:3; "naro "-~7j "n-00 or zoro
Convorging With oach othor; soma rf"Dzdo~-- "-~'-.vo a voz-.1 C'-ico,
LO
~s; owls). An atlas issued rac-ont has novo.-al *AUrACIz';"d ~Acturco of th3so dinto-.~Cd
ow Uly
n
3, lw:ios. rfha shapri of somo of thc~;;-. co-Old b,) -J'.Oni:;Gd
But thoso galadoa had no Cas. I~vovaz, all azo noz'
ox-mationo. One of tLo grrair-;doz; is cn-.~ocially ' -A t ti0 n r 0 3
A L
tha =ain bodio:j of tva convoz~;cd a~,d- t'.-,3i:: t--,JLI---- lb,~:atu 1--'I'M 'UwD of W--toz
L
in tho Sofpor whool. ilho photos of t-o r-~-Aal' 1,.32, ,L~ca was
souroe of olrvatod zadllo c-mmission, ehowcd flov3 of inca;-.'Os Oor't
Oru-otin'? 1n) -,-,a Cova, 'Iho oruptlion -inorati-.6--r th3 flo,.%; occu,---,zd in. T,1-13 co;:,~ o-
lazq 1.5 =I-Ilion yoars a.-p and w---- --Uch zara powar2ul t,:aar. ovor obsorvcd in th 3
evan in Su:;a;:--Ova Stars. Tho fact of this t-.at '-:2= '..;u v I n
-Y
two radiation centors woza a----o fo.=.cd 'by c-.~--Ilosio-A. I.-I conc'-IU3:~on,
tWo quastions: (1) tho farthont Imoum obj-3ct 13 A".xz-1LICd ua C.T' C~ 0--'
oi&it billion liZ;!it yC';ar:;; (2) t~i3 problcm of -.-o racossion of intoractizz: C: 03 --~3
Still -I;.Is01VOd.
SUB COLO: 03/ SUBM DiM: 22k)r~~6

SUAKIN, N.K.; VOROHTSQY_~VM~TAMINOV, B.A. ,prof... red.;. WSIKOV.
G.G., red.; HOV053i~ffi,"V. f._,___f"ikhn. red.
[Teaching astronomy in schools; collected articles] Prepodavanie
astronomli v shkole; ebornik statei. Pod red. B.A.Vorontsova-
Velliaminova. Moskva, 1959. 269 p. (MIRA 13:2)
1. Akademlys pedegogicheakikh nauk RSM, Moscow. In3t-tut metodov
obuchenlya. 2. Laboratoriya metodiki fisiki Institute metodov obu-
chaniya Akademii pedegogichaskikh nauk RSFSR i Shkols No.500 g.
Kosk-Ty (for Semakin). 3. Chlen-korrespondent Akademii pedegogicheskikh
nauk RSM i Pedinstitut imeni V.P.Potemkina. g.Moskva (for Vorontsov-
Vellyaminov).
(Astronomy--Study and teaching)

VOROIMTSOY-YELITAMINOY, Boris Aleksandrovich; KARTTNOT, D.Ts., prof.,
-- ie~~
seniiint:4-~]=O"- ,
9 red.; BRIMNO, K.F., takhn.red.
[Assays about the universe] Ocharki o vaelennoi. Izd.4.
Moskva. Goo.izd-vo fiziko-matem.lit-ry, 1959. 532 p.
(KMA 13:2)
(cosmogony)

VORONTSOV-1i'EL'YfiMINOV, B,,P.
------ - -. ~,
'EvIrlinces of magnt cialill.0 phfnozera in the stzucl,um clr
I
gga-axLes. Astt-on.,~hur. 41 -3-') 164.
.1. Go,-udaratvarnyy Iri3titut, lr,. F.K.Shtarnberga.
(M f TU. j 7, ILO)

u Pa L4 i-ae - - r
tk vo-US
?Y YUILu.Lv
uuu- interactIngy
i,4A
RM2
IM, 4A
160
Ll o
ut
TER. IN

- C - -- t , , -
.12

REYSff, Arvid Karlovich; T otv.red.;
KOLOKITTSEV, A.D., red.izd-va; KOROVMMOVA, Z.A,, tekhn.red,
(Lubrication of strip mining machinery: handbook] Smazka mashin
ugollryich karlerov; spravochnik. Moskva, Ugletekhizdat, 1959.
213 'P. (KIRA 12:11)
(Lubrication and lubricants)
(Coal mining machinery--Kaintenance and repairs)

YORCHTSOV-yn'TAKINOT, Rikolay Pavlovi.0, doteent; SHAGINOV, Dmitriy Luklya-
novich. dotsent; PX=V, Kikol.ey Mitrofenovich, dotsent,, Priniusl
uchastiye PMW. R.N., dotsent. DOMOYSKIT, N.G., prof., doktor
takhn.nauk, red.; BWY, B.A.., inzh.p nsuchnyy red.; RITSH, A.K,, Inzh.,
nauchnyy red.; UDOD, V.Ye.9 red.izd-va; HAUMOVA, G.D., tekhn.red.
[Building machinery-, album of drawings] Stroitelinye mashiny; allbom
chertezhei. Pod red. H.G.Dombrovskogo. Moskva, Gos.izd-vo lit-ry po
stroit., arkhit. L stroit. materialam, 1960. 5 p. 294 p. of diagre.
(MIRA 13:12)
1. Kafedra "Stroitellnyye maahiny* Moskovskogo ordene Trudovogo Kresnogo
2nameni inzhenerno-stroitellnogo institute imeni V.V.Kuybyaheva (for
Toronteov-Vellyaminov. Shaginov, Petrov). 2. Voyanno-transportnoya
akademiya (for Popov).
(Building machinery)

VORONTSOV-VICLOYAKINOV. Nikola-_Pavlovich, kand.tekhn.nauk- PULIKAHOV,
Hikolay Viktorovich, kand.tekhn.nauk; RYAXHIN, Vi;tor
Alaksandrovich, kancl.takhn.nauk; PODOBIW, B.G., red.; PXLSO,
U.N., takhn.red.
[Assistant operator of diesel and electric construction
excavators] Pomoshchnik mashinists dizelInykh i elektri-
cheskikh stroitellnykh ekskavatorov. Izd,2,, perer, i dop.
Pod obahchei red. N.P.Voronteava-Velliaminove. Koskva, Vass.
uchabno-pedagog.izd-vo Proftekh12d8t. 1960. 439 p.
(MIRA 13112)
(Bxcavating machinery)

RiEysH, Arvid Karlovich; VORONTSOV-VELIMINOV., II.P.,, nauchrqy red.;
YAAL,U,IOVSKIY, Yu.F;-_WV_Aj L.M.# tekhn. red.
., red.; IIESHY6
[Single-bucket construction excavators] Odnokovshovye
stroitellnye ekskavatory. Kalinins Proftekhizdatj 1961,
100 plates. (Excavating machinery) (MIRA 15:3)

YORONTSOT-VILITA)(NOV, N., kand.takhn.nauk
Rotary excavator. ;Untekh. 4 no.M-10 Ag 160.
(Kim 13:9)
(2xcavating machinery)

pavlovicb; FULIMMOV- Ilikolay
LO 1
~V yAg Viko
; 1 33 eksndrovich; REYSHJ,
vT NEL~4 ~OV~ r
r
r h~
V r ch; ved, red-
AK.--,'-naucbn. red.; BEUZOVSKkyiy A,L.j st ekska-
r of agricultura3. excavators' Maebini
[operato 0 khoziaietva. Moskva, Vysshaia
vatorov diia sell-skog (MIRA 18:7)
sbkolas 1965. 399 P.

YORONTSOV-VELIYAMINOV, P.N.; NOVIKOV, V.V.
Propagation of an electromagnetic pulse over a plane nommiforn
track. Probl.dif.i raspr, voln, 23158-165 162 , (KRA 16SO
(Electromagnetic waves)

~u
lyfim,
cl N11
fill
v !-j
hi
r. . 'A I I j P:,:,
-JIH - A I i 1 1. A ~j
]I! ail- 0.3 . ~ . I?
a,,
p,
"r,!i N's
AS

FEDOSENKO, Radiy Yakovlevich;VORONTSOV, F.F., red.
(Transformers in lo0al, electric power distribution networks]
Transformator v mestnoi, rasprodelitellnoi elektricheskoi seti.
Moskvap Izd-vo M-va kom=n.khoz.RSF,-R, 1963. 83 p.
(MRA 17:3)

ACC, Nit: AP60?,135'1 SOURCECUDE: UR/Z1Z9?/66/0G0/003/CjG? 1 /0021
AUTHOR: Z -akliarov, M. V. (Doctor of technical aclbriceS); Putsyh!r~, G. G.
(Candidate of technical sciences); Step~jr~ava, M. .,:(~:andi date of technical
sciences); Vorantsova, Lu.,A. (Engineer)
ORG: none
TITLE: Alloys for electric-machine ,commutators
dA
SOURCE: Elektrotckhnika, no. 3, 1966, 21-23
TOPIC TAGS.- electric machine, electric m"%ij1C.crjmi-n.utator, copper alloy
ABSTPACT: The results are reported of an cxperirnenfal inveptigatioa of high-
conductivity low-alloy ;,I Cu-M-Bc, ,Cu-Ni-:Ei~''r-u-Cr'-Zr)-tu-Cr-llg,
_Sopp~~rv. ' I ~'/ --, _ ;?
Cu-Cr-Be, Cu-Cr-Ti, Cu-Co-Be, Cu-26r-M, U-re; for control
U-zr
purposes, copper Ml-4. a copper' niagnesium-alloy, and Iff, -Cr bronzes
Card I /?, UDC: 669'.35.001.5

L 09937-67
ACC NR: APO'OZ1057
were also tested. The alloys were subjected to two ti~ea.'tnient.,!, (1) Watcr-quench
hardening at 960-980C and tempering at 470-480C S or '51irs; (2) The same
hardening, then 50% workharclening, and then tempeii:nA -at 470-480C for 4 hra.
Experimental curves and tabula"i,-_' data show that: their hardness, wear
resistance, heat resistance, anu: Llectric conductivit the following alloys can be
Y. 0
recommended for the commutators of elc'ctrical macdiin~qzy oincrating at "'50-50OC:
-a chrome -zirconium bronze containing.O.-Z5-0.57a Ci- and 0. 15-0.3511'o Zr (or its
cheaper substitute, chrome -magnesium bronze) and'a. nickel -beryllium bronze
containing 0. 8-1. 111o Ni and 0. 15-0. 25% Be. The sp,cond therma: treatment ir,
recomn. --nded for these bronzes. OrIg. art. has: 1 an"` ZI
SUB CODE:J 11, 09 SUBM DATE: none ORIG RET., 004- OTH PLEF: 005

nqye~!ichj__-C OV, B.I., r9d.; ISUPOVA, N.A.,
VORONTS fj__jqvgqaiy.A!~d- - HUMAN
takhn.red.
(Yalta; roference guidebook] 1AIte; putevoditall-opravochnik.
Simferopoll, Krrd2dat. 1960. 92 p. (MIRA 14:2)
(Yalta--Ouidobooks)

24M SOV/48-23-9-16/57
AUTHOR: Vorontso7k_)Le.
TITLE: Dependence of Total Intensity of Spectral Lines on
thin Concentration of Atoms In a PulsW Discharge
PERIODICAL: Izvestiya Akademii nauk SSSR. Seriya fiziohenkayn, 1959,
Vol 230 Nr 9, pp 1088-1091 (USSR)
ABSTRACT: In the first part of the present paper the methods and the
selection of experimental conditions are discussed. In this
investigation a method for a forced introduction of electrode
material into the spark space by pulsed discharge is dealt
with, in which case the discharge is localized on a certain
part of the test sample. As shown in an earlier paper (Ref 1)
by the author, the dimensions of the electrode holes in this
case remain unchanged in ordir to eliminate the selectivity
of the material entry into the spark apace and the influence
of "third" elements. The forced introduction of a certain
quantity of material is necessary for an investigation of
the interrelation between the total intensity of the spectral
lines and the concentration of the atoms. Figure 1 shows the
blackening along the line Si 2516 R in the silumin spectrum
Card 1/3 for various kinds of spark discharge and in the alternating

SOV/48-23-9-16/57
.~Dependence of Total Intensity of Spectral Lines on the Concentration
of' Atoms in a Pulsed Discharge
current are. The diagram in figure 2 shows the influence exer-
cised by the diameter of the localized perforation of the
test sample upon the slope of the calibration curves for
silicon in the case of soft discharge '/ and in figure 3 the
calibration curves for zinc at various working conditions.
It is found that in a hard discharge the calibration curve
taken a rectilinear course. Also the influence exercised by
.the hole dimensions in the electrode surface upon ~he material
leave . depenling upon the sample composition is investigated.
It was found that, in the caae of a hard discharge, the radia-
tion atoms are distributed nearly uniformly within the dis-
charge zone. In the second part of the paper, the total
intensity of the spectral lines depeading upon, atom concen-
tration in a hard pulse discharge is investigated. Figure 4a
shows 'the calibration curvea for the determination of zinc
in copper and bronze within the range of 0.39-62~, and the
calibration curves for the determination of chromium in the
binary alloy Cr-11i in the range of concontration of 2-37~-
Figure 0 shows the corresponding theoretical curves for the
Card 2/3 case of complete absorption. The practical value of the present

SO'1/48-23-9-16/57
'Dependence of Total intensity of Spectral Lines on the Concentration
of Atoms in a Pulsed Discharge
paper is the theoretical possibility of obtaining calibration
lines with an inclination of 45 , which is possible in the
case of spark spectral lines up to comparatively high concen-
trations. This may be realized in the analysis of steel,
silunin, and brass. There are 5 figures and 1 Soviet referenoe.
Card 3/3

"--~AO~NTSOV Yo.S., kand.te':jin.-la-,l-?c,' 3~*-Ir,:.",
dok-t-or-Te-Tam. riauk,
Mass transfor of iron, SU7
Trudy Ural. o1
rMass tmnsfer) OA4, -ld
(%a,!-!.ol3ot-)!

L o4go6-67 r3W (d)/EWT(1)
UR K_C6D9-_tfR7d0_6_0T676 1--- 16
_AC27Z ~AT650_22684 7V060T
__S-61M0k__C6tF9-_tfR 66/000/000/016YA16
~I I'~ fc 10 ~GD 0 _0~070_0 07~~o
0
AUTHOR: Var6havs!&. V. I Vorontsova,_ 1. P.
ro~
ORG: none
TITLE: The use of qVhastio automatons of variable structure to solve.cortain behavior
problems
SOURCE: Moscow. Institut avtomatiki I telemekhaniki. Samoobuohayunhehiyesya
avtomaticheskiyo si~_temy matle''_ s-y-Btems), MoscIow, Izd-vo Nauka, 1966'.
158-164
TOPIC TAGS: game theory, stochastic process, finite automaton
ABSTRACT: The authors a nalyze some behavior problems for variable -structure stochastic
automatons in game situations. The dofinitions and notation adopted In the paper are those of
M. L. Tsetlin (e.g., Konechnyye avtomaty I modenrovanlye prosteyshikh form povedenlya.
--UMN, 1963, vol. XVIII, vyp. 4 (112)). The zerc-sum game of a variable -structure auto-
maton with a single opponent using one pure strategy is considered In an effort to demonstrate
the conditions for asymptotic behavior optiijaality of such an automatic device in a stationary
random environment. The simplest stochastic automaton version is Considered, i.e., the line--t
ard 1/2

L 04906-67
[XtCRRs AT6022684
automaton without Input. Expressions are derived for Lhe mathematical win expectancy of such
I
an automaton (Ck). Games by two such Ck automatons are considered for pure strategies,
state diagrams are analyzed, and experimental data on Ck automaton assignment game behavI r
are presented. In Uic case of the nonstatlonary (random) environments (to,%rh1ch the problem
of Inter-automaton gaming can ultimately be resolved) It Is not yet possible to formulate re-
quirements as the method of changing the state transitioif probabilities. It Is also shown that
a Ck automaton which has functioned for any extended period of time In one stationary medium
Is very slow to retrain Itself for operation In another enitronment. The elimination of this
defect is seen as the k~y to the ~esiga of an automaton capable of optimal behavior in nonsta-
tionary environments. The authors wish, In conclusion, to express their sincere gratitude to
M. L. Tact , 1. 1. PyatgtjkIv--ShaW o, V. Yu. Krylov, S. L. Ginzburg. and V. A.Volkons)d
for their willingness to take part In a discussion of the problems considered In this paper and
for their many helpful. suggestions. Orig. art. has: 2 figuris, 3 tables, and 9 formulas.
SUB CODE: 09,12/ SUBM DATE: 02Mar66/ ORIG REF: 008
'I Card 212

VORONTSOVA, Ye.l., doktor med. nauk,, red.
[Industrial lorgiono and safoty menouron for electri:! welding
operations; collection of transactions of the scivrit fic
conference on March 29-30, 19601 Gigiena truda I, tbkMilka bez-
opaBnosti pri elektroavarochnykh rabotakh; sbornik trudov na-
uchnoi konferentsii 29-30 marta 1960 g. Pod red, E.I.Vorontsovoi.
Moskva, In-t gigierW truda i profzaboloyanii WIll SSSHI 1962.
142 p. (HIRA 17:4)
1. Ilauchno-tekhnicheakoye soveshchaniye po voprosam giglyeny
truda i tekhnike bezopasnosti pri elektrosvarochnykh rabotakh,
Moskvaj 1960.

VORONTSOVA, Ye.I., doktor med. nauk; ALEKSEYEV, Ye.K., inzh.
Conference on labor hygiene and safety in electric
welding operations. Svar. proizv. no.5143-45 Yq 164.
(MIRA 18ill)

V.ORONTS n-T-,,doktor med. nauk; 7TSMF.NITSKIY, D.I., inzh.
Consultations on questions asked in our readers' letters. Svar.
proizv. no.8:48 Ag 164. (IMTRA 17:9)
1. Institut gigiyeny truda i professionallnykh zabolevaniy AMN SSSR
(for Vorontsova). 2. Vsesoyuznyy nauchno-issledova tell skiy institut
avtogennoy obrabotki metallov (for Te=enitskly).

VOPIORTSOVA, YC.I.; SH17-:0KOV, YU.G.
Some aspects and prinei.rial tasko (,-T indunt-r-ii-d in re2Atlcr
to the development of 1,:(,Pvy cl-lemical indus"'ry. Vest. A~l 3:;S-- 1~)
no.7:3-8 164. (14:11"'. 1F:3)
1. Inatitut r,,J~,Iyeny tr~,,:a .1 :,abolevarl.y 8Ssr,,
Hosk
va. -

VORONT6OV, Ye* S. Cand Tech Sci -- (diss ) "Diffusion in molten alngs."
Sverdlovsk, 1958. 14 pp (Min of HiZher Ediaontion USSR. Ural PolytechnIc
I S I
Inst im A. .1. Kirov), 100 copies M, 14-58, 113)
-51-

M
L 47392-66 EWT(d)/FSS-2
ACC NR, AP6031030 SOURCE CODE#' TJR/0109/66/011/009/1657/1665
AUTHOR, Vorontsov,, Yu. 1. ; Polyakov, J. V.
ORG- none
TITLE: Investigation of continuous iieals i lines with nonlinear resistance
SOURCE: Radiotelihnika I elektronika, v. 11, no. 0, 1966, 1657-1665
TOPIC TAGS: signal propagation, continuous signal, nonlinear resistance line,
signal propagation velocity, signal shape
ABSTRACT: The propagation of continuous signals in lines with nonlinear resist-
ance is investigated. It is shown that the resistances existing in the series and
parallel branches of the equivalent circuit of such a line affect continuous signal
propagation in an essentially different manner. Simplified equivalent circuits
used in earlier studies have failed to provide a complete picture of all the types of
continuous signals possible in such a line. Conditions of the applicability of
simplified equivalent circuits are established, Conditions for the existence of
continuous signals and the dependence of their shape and propagation velocity on
circuit parameters have been determined. It is demonstrated that with a specific
1/2 UDC! 621. 372. 2

1 47392-66
P6031030
A
relationship of parameters, depending on the displacement current, two types of
stationary signals propagating at completely different velocitie's are possible in
9 itle
these lines. Orig. art. has: 6 figures, 22 formulas, and a biblio raphy of 6 title
[Authors' abstract] IDW]~-
SUB CODE: 09/
SUBM DATE: 05May65/ ORIG RLIF: 0051 OTH REF: 001
ccid 2/ 2

SOV, YU.N., MOROZOV. M.G.
VALOV VORM oscacorwl-
.............. .* lash tims lOss than a micr
j~wk ignition unit with a f l6o. (MIRA 13:
.2:122-123 W-AP
Prib.l. takh-ekBPG no aledovatel'Bkiy Iektrokeramicheskiy institute
1. GoaudaretvOUDU is ge lighting)
(Alectric dischar

83636
S10291601000100910031008
B013/Bo6o
AUTHOR: Vorontsov-Vel! Professor
"W~
n Universal Validity?
TITLE: Has the General Law of Gravitatio
PERIODICAL: Tekhnika molodezhi, 1960, No. 9, pp. 10-13
TEXTj The author contributes the present article in response to reader's
A. Viskovatava, of Chardzhou, Turkmenskaya SSR, desire to hear about new
theories oii--i-he unlimited validity of Newtonfs law of gravitation. The
author starts by pointing out that attraction depends on the size of a
system. He confronts microcosmos with megaeosmos, and gives their
respective orders of magnitude. It was possible to establish the pre-
dominance of Newtonts law of gravitation in the megacosmos. Up to date,
this law has been unrestrictedly extended to all phenomena arising within
galaxies and their interrelations. In fact, this law has b_qen verified
only with respect to double and, at most, multiple starsYffegarding the
clustering of several dozens of stare, no proof has as yet been obtained
as to whether there are other types of interactions comparable to the law
of gravitation. Conceptions and theories applying to the solar system,
Card 1/3

'83636
Has the General Law of Gravitation Universal S/029/60/000/009/003/008
Validity? B013/BO60
and even to microcosmos, are often used to explain the formation, evolu-
tion, and interaction of stellar systems. Since, however, only the form
of stellar systems, but not the processes occurring in themp are observed,
it is not possible to prove the validity of the theories applied to them.
The photographic stellar atlas published by the Observatory of Mount Palcmar,
USA, is systematically studied in the USSR.As many as 500 galaxies,
designated as interacting, have already been identified. These comprise
pairs and groups of galaxies, whose normal form is visibly distorted, but
also such as are situated in a common bright nebula. The author gives
some proofs for the fact that interactions of these pairs and groups of
galaxies have no gravitational characterp and that the form distortions
have nothing to do with ordinary attractive effects. Arguments have also
been put forward in favor of the proposition that galaxies possess a high
toughness. This can be hardly explained by interstellar gravitation.
Rosearch made into the interactions of stellar systems led to the belief
that also othert as yet unknown, forces exist In these systems apart from
gravitation about which there is no doubt. Academician V. A. Ambartsumyan
indicates a number of convincing arguments for his hypothesis thWt___fF_e___
centers of some galactic clusters oplit and fly asunder to form now
Card 2/3

83636
Has the General Law of Gravitation Universal s/o2g/60/000/009/003/008
Validity? B013/BO60
galaxies. The author assumes that individual members of interacting
galactic clusters arise simultaneously, and mutually disturb their
normal evolution. In flying asunder, they exert an inexplicable effect
on each other. Physicist N. P. Lebedevis mentioned. There are 11 figures.
Y
Card 3/3

YOROFfSOV-VBLIYAHINOV, B-A-
Interaction of galaxies and the nature of their arms, bars,
and tails. Morphology of qtlaxtbs: part 5. Astron.zhur,
35 no.6:858-868 X-D 158. (MIRJk 11: 12)
1. GosudaretvanVy astronomichookiy inatitut imeni P.1*
Shternberg%. (Oklaxies)

TcROBTSOT-TAIUMINOT, Boris Aleksandrovichl TWYM, N.P., red.;
(Ocatchas of the hist of astronomy in the U.S.S.R.) Ocherki
9ry
istoril astronomii v SSSR. Koskva, Goo.izd-vo fitiko-matem.
lit-ryt 1960. 227 P. (XM 14:3)
(Astronomy) I

VORON,TSOV-VELITA14INOV, B -# prof*
:A
.Is the universal eravitation, lav really, universal? Tekh-mol. 28
no*9110-13 160, NDU 13:10)
(Gravitation) (Galaxies)

VORONTSOV-TELITAMINOV, B.A.
I,-.
Partial gae'deasities in Wtipplele comet (1942g). Astroa.zhur.
37 no.4:709-70 JI-Ag 160. W" 13:8)
1. Gosudaretyennyy antroaomichookly institut im. P.-K.Shternbarga.
(Comets--1942)

,_VORONTSOY-VILITAMINOV, B.A.
Problem of comparing the dimensions of 9alaxt65- Antroo.zhur-
37 no.4:7?&-?80 JI-Ag 160. (MIRA 13:8)
1. rjosudaretvanVy astronomLehaskV institut im. F.K.Shternberga
(Galaxies)

87248
S/033/60/037/oo6/007/022
7 7) B032/E514
AUTHOR: Vorontsov-Vellyaminov. B. A.
TITLE: Variations in the Spectrum of the Planetary Nebula
IC4997 and Their Origin
PERIODICAL:Astronomicheskiy zhurnal, 1960, Vol-37, No,6, pp.994-1000
TEXTt Aller and Liller (Ref.1) have noted variatio!ts in the
relative intensities of the lines H and X4363 (0111) ill tile
spectrum of IC 4997 as reported by Ydifferent workers. They have
suggested that the reduction in the intensity of the line X 4363
is due to a reduction in the electron density. The problem has
been discussed theoretically by Gurzadyan (Ref.2). However,
Gurzadyan erroneously assumed that in the first observations of
iqi6 the line X4363 was twice as bright as H . The present
author gives a detailed discussion of the ratio of the intensities
of the lines X4363 and H using existing observations as well as
additional data based onymeasurements on a standardized spectrogram
obtained by M. V. Savellyeva on September 5, 1959. This spectro-
gram was obtained using an objective prism and the 50 cm Maksutov
camera at the Crimean Station of the Shternberg State Astronomical
J
Card 1/5

87248
S/033/60/037/006/007/022
E032/E514
Variations in the Spectrum of the PlAnetary Nebula IC 4997 and
Their Origin
Institute (GAISh). Agfa ISS plates were used. The exposure was
2 1/2 hours and the dispersion 200 A/mm at H (further details
will be published in a later paper). The spectrx9ram obtained on
June 2, 1960 confirmed the 1959 results. Other data employed in
the present discussion were as follows:
Date and Observer X 43630-H
1916, September, Wright (Ref-3) 1.1
1938, August, Aller (Ref.4) 1.6
1940, June, Struve apd Swings (Ref-5) 1.2
1949, Aller (Ref.1) 1.0
1956, Aller (Ref.1) 0.77
1950, September, Savellyeva and
Vorontsov-Vollyaminov o.61
The case of IC 4997 is said to be exceptionally favourable, since
the intensities of the lines X 4363 and H are almost equal
and it is quite clear from the spectrum whicliyof them is stronger.
Card 2/5

87248
S/033/60/037/oo6/007/022
B032/E514
Variations in the Spectrum of the Planetary Nebula IC 4997 and
Their Origin
In 1916 the intensities of these two lines were practically equal,
in 1938 to 1940 X 4363 became appreciably stronger, while in 1956
to 1959 it was appreciably weaker than H There is thus little
doubt that the ratio of the intensities Xi the two lines does, in
fact, oscillate rather than systematically decrease. An attempt
was made by the present author to evaluate the values of N and
Te simultaneously, using the Seaton method (Refs. 10 and 117.
However, this attempt was unsuccessful owing to the lack and low
accuracy of observational data and the approximations made in the
theory. The IC 1997 nebula has exceptionally high values of N
namely, 105 _ 3.09 and the approximate equations apparently do e
not hold for this nebula. The surface brightness of the nebula
in HP In absolutemunits and the photographic magnitude of the
nucleus (about 13.7) were obtained directly from the spectrum.
The decrease in the intensity of X1063 is said to be probably due
to a drop in the temperature of the nucleus. In general, this
temperature probably oscillates. Observations can also be
Card 3/5

87248 ,
S/033/60/037/006/007/022
E032/E514
Variations in the Spectrum of tho Planetary Nebula IC 4997 nnd
Their Origin
explainedqualitatively by assuming that an increase in the corpus-
cular emission of the nucleus takes place. The nucleus belongs
to the Wolf-Rayet type and the enhanced corpuscular emission leads
to an acc.%Ierated supply of oxygen to the envelope. The observed
change in the electron temperature of IC 4997 could be due to an
increase in the concentration of oxygen by anything between 0.02
and 0.06 5with a change in the relative abundance from 1:5 x lo5 to
315 x 10 - If the mass of the envelope of the nebula is 0.01M
then this process will require an increage in the injection of 0
oxygen from the nucleus of about 2 x 10- M per year. For normal
Wolf-Rayet stars, the mass loss by ejectionois estimated as 10-5 M
per year, i.e. a quantity which is greater by three or four 0
orders of magnitude than the above figure. In usual stars the
amount of oxygen is less than the amount of hydrogen by a factor of
1000. However, it is considered that Wolf-Rayet 5stars are very
poor in hydrogen and hence if they lose about 10 M per year,
the fraction of oxygen should be greater than ItIO009 It follows
Card 4/5

8 18
S/033/60 OM/Oo6/o07/022
E032/E514
Variations in the Spectrum of the Planetary Nebula IC 4997 and
Their Origin
that the observed decrease in the electron density could be explain-
ed by a much smaller increase In the corpuscular emismion from the
nucleus. Since, however, there is no progressive chang*e in the
spectrum of IC 4997 and only oscillations appear to be present,and
since in the case of NGC 6905, for example, an increase in the
temperature of the nucleus has been observed, it is more probable
that an oscillation in the temperature of the nucleus of the
IC 4997 nebula does in fact occur,and changes in the chemical
composition of the envelope of this nebula are not significant in
this connection. There are 23 references: 5 Soviet, 18 non-Soviet.
ASSOCIATION% Gos. astronomicheskiy institut imeni P. K. Shtern-
berga (State Astronomical Institute imeni
P. K. Shternberg)
SUBMITTED: may 2o, 196o
Card 5/5

RAYSH, Arvid Karlovich; I P , otvatstvennyy redaktor;
Y. A.D.-O-re"ktor isdai's Ostia; DOVA, Ts4o, takhnioho-
skiy redaktor
Clubrication systems of single-bucket excavators] Sistemr smaski
odnokovehavykh skskayatorov., Moskva, Uglatekbizdat, 1956o 124 p.
(MIRA 10:1)
(11xcavating machinary-Iubrication)