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EZ to evolve ZAMS stars: A program derived from Eggleton's stellar evolution codePAXTON, Bill.Publications of the Astronomical Society of the Pacific. 2004, Vol 116, Num 821, pp 699-701, issn 0004-6280, 3 p.Article

DIE ENTWICKLUNG DER STERNE. = L'EVOLUTION DES ETOILESKIPPENHAHN R.1975; NOVA ACTA LEOPOLD.; ALLEM.; DA. 1975; VOL. 42; NO 218; PP. 115-134; BIBL. 19 REF.; (EVOL. JAHRESVERSAMMLUNG. VORTR.; HALLE (SAALE); 1973)Conference Paper

Solving the Giant Stars Problem: Theories of Stellar Evolution from The 1930s to The 1950s = Résoudre le problème des étoiles géantes : Les théories de l'évolution stellaire de 1930 à 1950CENADELLI, Davide.Archive for history of exact sciences. 2010, Vol 64, Num 2, pp 203-267, issn 0003-9519, 65 p.Article

The effect of back pressure on the contact evolution of a close binary systemNAKAMURA, M; NAKAMURA, Y.Astrophysics and space science. 1986, Vol 118, Num 1-2, pp 283-286, issn 0004-640XArticle

Stellar evolution at high mass with convective core overshootingSTOTHERS, R. B; CHAO-WEN CHIN.The Astrophysical journal. 1985, Vol 292, Num 1, pp 222-227, issn 0004-637XArticle

The outcome of accretion on to a fully convective star: expansion or contraction?PRIALNIK, D; LIVIO, M.Monthly Notices of the Royal Astronomical Society. 1985, Vol 216, Num 1, pp 37-52, issn 0035-8711Article

Les enveloppes circumstellaires vue en radio (masers OH) et par les observations infrarouges (IRAS) = Circumstellar envelopes seen in radio (OH masers) and in the infrared (IRAS)David, Pedro; Le Squeren, Anne-Marie.1992, 197 p.Thesis

Bounds on hadronic axions from stellar evolutionRAFFELT, G. G; DEARBORN, D. S. P.Physical review. D. Particles and fields. 1987, Vol 36, Num 8, pp 2211-2225, issn 0556-2821Article

Evolution de pulsarsGUSEJNOV, O. KH; YUSIFOV, I. M.Astronomičeskij žurnal. 1986, Vol 63, Num 2, pp 265-273, issn 0004-6299Article

A simple model for binary star evolutionWHITE, C. A; EGGLETON, P. P.Monthly Notices of the Royal Astronomical Society. 1985, Vol 214, Num 3, pp 357-378, issn 0035-8711Article

Nouvelle évidence pour la perte de masse dans les céphéides classiquesSTIFT, M. J.Astronomy and astrophysics (Berlin. Print). 1984, Vol 140, Num 2, pp 445-448, issn 0004-6361Article

EVOLUTION OF HELIUM RICH STARS WITH HYDROGEN BURNING.ROSER M.1975; ASTR. AND ASTROPHYS.; GERM.; DA. 1975; VOL. 45; NO 2; PP. 335-341; BIBL. 14 REF.Article

THE EVOLUTION OF A CONTACT BINARYHAZLEHURST J; MEYER HOFMEISTER E.1973; ASTR. AND ASTROPHYS.; GERM.; DA. 1973; VOL. 24; NO 3; PP. 379-392; BIBL. 29REF.Serial Issue

LES BINAIRES SERREES ET LEUR SIGNIFICATION POUR LA THEORIE DE L'EVOLUTION STELLAIREMARTYNOV D YA.1972; USP. FIZ. NAUK; S.S.S.R.; DA. 1972; VOL. 108; NO 4; PP. 701-732; BIBL. 3 P.Serial Issue

MASS LOSS IN EARLY STAGES OF STELLAR EVOLUTION.DEARBORN DSP; KOZLOWSKI M; SCHRAMM D et al.1976; NATURE; G.B.; DA. 1976; VOL. 261; NO 5557; PP. 210-211; BIBL. 30 REF.Article

POSSIBILITY OF SYNTHESIS OF PROTON-RICH NUCLEI IN HIGHLY EVOLVED STARS II.ARNOULD M.1976; ASTR. AND ASTROPHYS.; GERM.; DA. 1976; VOL. 46; NO 1; PP. 117-125; BIBL. 43 REF.Article

NON-EXPLOSIVE MASS LOSS.WOOLF NJ.1974; INTERNATION. ASTR. UN., SYMP.; NETHERL.; DA. 1974; NO 66; PP. 43-255 (15P.); BIBL. DISSEM.; (LATE STAGES STELLAR EVOL. COPERNICUS SYMP. V; WARSAW; 1973)Conference Paper

POST MAIN SEQUENCE EVOLUTION OF SINGLE STARS.IBEN I JR.1974; ANNU. REV. ASTR. ASTROPHYS.; U.S.A.; DA. 1974; VOL. 12; PP. 215-256; BIBL. 4 P.Article

WIE STIRBT EIN STERN. = COMMENT MEURT UNE ETOILE1973; ORION; SUISSE; DA. 1973; VOL. 31; NO 134; PP. 12-13Serial Issue

ON THE CONDITIONS FOR HOMOGENEOUS STELLAR MODELS TO HAVE ONLY REAL SECULAR EIGENVALUESGABRIEL M; NOELS A.1972; ASTR. AND ASTROPHYS.; GERM.; DA. 1972; VOL. 20; NO 3; PP. 455-459; BIBL. 13REF.Serial Issue

ICI NAISSENT DES ETOILESWENZEL W.1972; REV. IENA; ALLEM.; DA. 1972; NO 7; PP. 319-321Serial Issue

LES STADES EVOLUTIFS DE QUELQUES SYSTEMES BINAIRES SERRESGALKINA T; RODIONOVA G; YUNGEL'SON L et al.1972; ASTR. SOVET AKAD. NAUK S.S.S.R., NAUCH. INFORM.; S.S.S.R.; DA. 1972; NO 23; PP. 82-84; ABS. ANGL.; BIBL. 12REF.Serial Issue

PRELIMINARY RESULTS ON DETAILED HELIUM SHELL FLASH CALCULATIONS.CHRISTY SACKMANN IJ; PACZYNSKI B.1975; MEM. SOC. R. SCI. LIEGE, 8.; BELG.; DA. 1975; VOL. 8; PP. 335-355 (20P.); BIBL. 17 REF.; (PROBL. HYDRODYN. STELLAIRE. 19E. COLLOQ. INT. ASTROPHYS.; LIEGE; 1974)Conference Paper

THE AFTERCLAP OF DEGENERATE CARBON IGNITION.BUCHLER JR; MAZUREK TJ; TRURAN JW et al.1974; COMMENTS ASTROPHYS. SPACE PHYS.; U.S.A.; DA. 1974; VOL. 6; NO 2; PP. 45-55; BIBL. 1 P. 1/2Article

DESTRUCTION OF THE S PROCESS (NSIGMA ) CORRELATIONS BY ELECTRON CAPTURE AFTER NEUTRON IRRADIATION.ARNOULD M.1972; ASTR. AND ASTROPHYS.,; GERM.; DA. 1972; VOL. 21; NO 3; PP. 401-412; BIBL. 41REF.Serial Issue

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