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THE EVOLUTION OF A 15 M CERCLE. STAR.CHIOSI C; NASI E.1974; MEM. SOC. ASTR. ITAL.; ITAL.; DA. 1974; VOL. 44; NO 4; PP. 665-670; ABS. ITAL.; BIBL. 7 REF.Article

EVOLUTION DES ETOILES DE MASSE INTERMEDIAIRE EN ROTATION DIFFERENTIELLE RAPIDETUOMINEN I; MUZYLEV V.1974; ASTR. SOVET AKAD. NAUK S.S.S.R., NAUCH. INFORM.; S.S.S.R.; DA. 1974; NO 33; PP. 48-71; ABS. ANGL.; BIBL. 20 REF.; (KRON. SOVMESTNOGO SOV.-FR. SOVESHCH. PROBL. FIZ. EHVOL. ZVEZD; MOSKVA; 1974)Conference Paper

DYNAMICAL PHASES OF ROTATING SUPERMASSIVE STARS.FRICKE KJ.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 189; NO 3 PART. 1; PP. 535-542; BIBL. 15 REF.Article

INFLUENCE OF OPACITY ON THE PULSATIONAL STABILITY OF MASSIVE STARS WITH UNIFORM CHEMICAL COMPOSITION. II. MODIFIED KRAMERS OPACITY.SASTRI VK; STOTHERS R.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 193; NO 3 PART. 1; PP. 677-678; BIBL. 9 REF.Article

EVOLUTION OF SINGLE STARS. VII. EVOLUTION OF MASSIVE STARSZIOLKOWSKI J.1972; ACTA ASTR.; POLOGNE; DA. 1972; VOL. 22; NO 4; PP. 327-374; BIBL. 1 P.Serial Issue

MAIN SEQUENCE MODELS FOR MASSIVE ZERO-METAL STARS.CARY N.1974; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1974; VOL. 31; NO 1; PP. 3-10; BIBL. 18 REF.Article

EVOLUTION DES ETOILES DE 16 M CERCLE., 32 M CERCLE., 64 M CERCLE.. IV. EVOLUTION DES ETOILES 16 M CERCLE. ET 32 M CERCLE. D'HYDROGENE-HELIUM PURVARSHAVSKIJ VI.1974; ASTR. SOVET AKAD. NAUK S.S.S.R., NAUCH. INFORM.; S.S.S.R.; DA. 1974; NO 33; PP. 72-78; ABS. ANGL.; BIBL. 7 REF.; (KRON. SOVMESTNOGO SOV.-FR. SOVESHCH. PROBL. FIZ. EHVOL. ZVEZD; MOSKVA; 1974)Conference Paper

EVOLUTION DES ETOILES MASSIVES AVEC ROTATION DIFFERENTIELLEMUZYLEV VV.1972; ASTR. SOVET AKAD. NAUK S.S.S.R., NAUCH. INFORM.; S.S.S.R.; DA. 1972; NO 21; PP. 11-24; ABS. ANGL.; BIBL. 15 REF.Serial Issue

EVOLUTION DES ETOILES MASSIVES AVEC SEMI-CONVECTIONVARSHAVSKIJ VI.1972; ASTR. SOVET AKAD. NAUK S.S.S.R., NAUCH. INFORM.; S.S.S.R.; DA. 1972; NO 21; PP. 25-45; ABS. ANGL.; BIBL. 25 REF.Serial Issue

ADVANCED EVOLUTION OF MASSIVE STARS. IV. SECONDARY NUCLEOSYNTHESIS DURING HELIUM BURNINGCOUCH RG; ARNETT WD.1972; ASTROPHYS. J.,; U.S.A.; DA. 1972; VOL. 178; NO 3, PART1; PP. 771-777; BIBL. 17REF.Serial Issue

ORIGIN OF COSMIC RAYS IN EXPLOSIONS OF MASSIVE STARS.SCHRAMM DN; ARNETT WD.sdIN: 13TH INT. COSMIC RAY CONF.; DENVER, COLO.; 1973; DENVER, COLO.; UNIV. DENVER; DA. S.D.; VOL. 1; PP. 646-651; BIBL. 1 P.Conference Paper

STABILITY OF SUPER-MASSIVE STARSFUJIMOTO MK; UNNO W.1973; PUBL. ASTR. SOC. JAP.; JAP.; DA. 1973; VOL. 25; NO 2; PP. 243-252; BIBL. 9REF.Serial Issue

ADVANCED EVOLUTION OF MASSIVE STARS. I. HELIUM BURNINGARNETT WD.1972; ASTROPHYS. J.; U.S.A.; DA. 1972; VOL. 176; NO 3, PART 1; PP. 681-698; BIBL. 31REF.Serial Issue

ADVANCED EVOLUTION OF MASSIVE STARS. II. CARBON BURNINGARNETT WD.1972; ASTROPHYS. J.; U.S.A.; DA. 1972; VOL. 176; NO 3, PART 1; PP. 699-710; BIBL. 32REF.Serial Issue

INFLUENCE D'UN MELANGE ADDITIONNEL SUR L'EVOLUTION D'ETOILES MASSIVESMASEVICH AG; POPOVA EI; TUTUKOV AV et al.1981; ASTR. SOVET. AKAD. NAUK S.S.S.R., NAUCH. INFORM.; SUN; DA. 1981; VOL. 47; PP. 31-37; ABS. ENG; BIBL. 12 REF.Article

EVOLUTION DES ETOILES MASSIVES ET PROBLEME DE LA SEMI CONVECTIONMASEVICH AG; TUTUKOV AV.1974; ASTR. SOVET AKAD. NAUK S.S.S.R., NAUCH. INFORM.; S.S.S.R.; DA. 1974; NO 29; PP. 3-26; ABS. ANGL.; BIBL. 3 P.Article

22NE (A,N)25MG REACTION IN CONE MANTLE OF MASSIVE STARS AT HIGH TEMPERATURES.KAKATI BN; DUORAH HL.1974; PRAMANA; INDIA; DA. 1974; VOL. 3; NO 2; PP. 89-94; BIBL. 13 REF.Article

ADVANCED EVOLUTION OF MASSIVE STARS. V. NEON BURNING.ARNETT WD.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 193; NO 1 PART. 1; PP. 169-176; BIBL. 21 REF.Article

PHOTOIONIZATION BY MASSIVE STARS IN PROTOGALAXIESTINSLEY BM.1973; ASTROPHYS. LETTERS; U.S.A.; DA. 1973; VOL. 14; NO 1; PP. 15-17; BIBL. 18REF.Serial Issue

CORE HELIUM BURNING IN MASSIVE STARSROBERTSON JW.1972; ASTROPHYS. J.,; U.S.A.; DA. 1972; VOL. 177; NO 2; PP. 473-488; BIBL. 43REF.Serial Issue

EVOLUTIONARY SCENARIOS LEADING MASSIVE STARS TO WR STARS: THEIR MUTUAL IMPORTANCE; THE ROLE OF MIXINGMAEDER A.1982; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1982; VOL. 105; NO 1; PP. 149-158; BIBL. 70 REF.Article

EVOLUTION OF MASSIVE CLOSE BINARIES. II. THE POST X-RAY BINARY STAGE: ORIGIN OF RUN-AWAY AND BINARY PULSARS.DE LOORE C; DE GREVE JP; DE CUYPER JP et al.1975; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1975; VOL. 36; NO 1; PP. 219-225; BIBL. 17 REF.Article

THEORETICAL STUDIES OF MASSIVE STARS. I. EVOLUTION OF A 15 MO STAR FROM THE ZERO-AGE MAIN SEQUENCE TO NEON IGNITION.ENDAL AS.1975; ASTROPHYS. J.; U.S.A.; DA. 1975; VOL. 197; NO 2 PART. 1; PP. 405-413; BIBL. 31 REF.Article

EVOLUTION DES ETOILES 16M CERCLE., 32M CERCLE., ET 64 M CERCLE.. III. EVOLUTION DES ETOILES 32 M CERCLE. ET 64 M CERCLE. AU COURS DES PHASES DE COMBUSTION DE L'OXYGENE ET DU CARBONE DU NOYAUVARSHAVSKIJ VI; TUTUKOV AV.1974; ASTR. SOVET. AKAD. NAUK S.S.S.R., NAUCH. INFORM.; S.S.S.R.; DA. 1974; NO 32; PP. 73-103; ABS. ANGL.; BIBL. 1 P.Article

STOCHASTIC MASS LOSS RATE FLUCTUATIONS AND EVOLUTION OF MASSIVE STARSNASI E.1982; ASTROPHYSICS AND SPACE SCIENCE; ISSN 0004-640X; NLD; DA. 1982; VOL. 85; NO 1-2; PP. 17-23; BIBL. 16 REF.Article

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