THE MASS-LUMINOSITY RATIO IN THE COMA CLUSTER OF GALAXIES FROM TWO-BODY INTERACTIONS.NOONAN TW.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 202; NO 2 PART. 1; PP. 551-557; BIBL. 13 REF.Article

MASSES OF THE DOUBLE-MODE CEPHEIDS AND THE MASS-LUMINOSITY RELATIONSHIPS OF CLASSICAL CEPHEIDSSAIO H; KOBAYASHI E; TAKEUTI M et al.1977; SCI. REP. TOHOKU UNIV., 1; JPN; DA. 1977; VOL. 60; NO 3; PP. 144-152; BIBL. 1 P.Article

ON THE RATIO OF MIXING LENGTH TO SCALE HEIGHT IN RED DWARFSCOX AN; SHAVIV G; HODSON SW et al.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 245; NO 1; PART. 2; PP. L37-L40; BIBL. 18 REF.Article

ON CORE MASS-LUMINOSITY RELATIONS FOR SHELL HELIUM BURNING STAGES OF STELLAR EVOLUTIONHAVAZELET D; BARKAT Z.1979; ASTROPHYS. J.; USA; DA. 1979; VOL. 233; NO 2 PART. 1; PP. 589-595; BIBL. 24 REF.Article

SPECKLE INTERFEROMETRY OF ETA ORIONIS.MCALISTER HA.1976; PUBL. ASTR. SOC. PACIF.; U.S.A.; DA. 1976-1977; VOL. 88; NO 526; PP. 957-959; BIBL. 10 REF.Article

WHITE DWARF STARSLIEBERT J.1980; ANNU. REV. ASTRON. ASTROPHYS.; ISSN 0066-4146; USA; DA. 1980; VOL. 18; PP. 363-398; BIBL. 4 P.Article

ELECTRONOGRAPHIC UBV PHOTOMETRY OF CLOSE VISUAL DOUBLE STARSPENNY AJ.1979; MONTH. NOT. R. ASTR. SOC.; GBR; DA. 1979; VOL. 187; NO 3; PP. 829-837; BIBL. 17 REF.Article

RELATION MASSE-LUMINOSITE DES NOYAUX DE GALAXIES ACTIFSDIBAJ EH A.1980; ASTR. ZH.; SUN; DA. 1980; VOL. 57; NO 4; PP. 677-680; ABS. ENG; BIBL. 18 REF.Article

THE INITIAL MASS FUNCTION AND STELLAR BIRTHRATE IN THE SOLAR NEIGHBORHOODMILLER GE; SCALO JM.1979; ASTROPHYS. J., SUPPL. SER.; USA; DA. 1979; VOL. 41; NO 3; PP. 513-547; BIBL. 2 P.Article

I. OBSERVATION DES ETOILES DOUBLES AU MOYEN DE LA CAMERA ELECTRONIQUE. II. ETOILES DE MASSES INTERMEDIAIRES DANS LA RELATION MASSE LUMINOSITE. III. ETOILES DOUBLES VISUELLES A LONGUE PERIODE.LAQUES P.1974; AO-CNRS-13396; FR.; DA. 1974; PP. (145P.); H.T. 39; BIBL. 8 P.; (THESE DOCT. ASTROPHYS.; PARIS VII)Thesis

QUASI-STELLAR OBJECTS AS ROTATING MAGNETIC SUPERSTARS. I: LUMINOSITY AND DENSITY EVOLUTIONSORRELL WH.1982; ASTROPHYSICS AND SPACE SCIENCE; ISSN 0004-640X; NLD; DA. 1982; VOL. 85; NO 1-2; PP. 3-15; BIBL. 32 REF.Article

CHEMICAL COMPOSITION OF UPPER MAIN SEQUENCE STARS. II. ECLIPSING BINARIES.SHIBATA Y; MIMURA K.1977; SCI. REP. TOHOKU UNIV., 1; JPN; DA. 1977; VOL. 60; NO 1; PP. 31-39; BIBL. 26 REF.Article

UBV PHOTOMETRY AND LIGHT CURVE SOLUTION OF THE ECLIPSING RS CVN BINARY SS CAMARNOLD CN; HALL DS; MONTLE RE et al.1979; ACTA ASTR.; POL; DA. 1979; VOL. 29; NO 2; PP. 243-258; BIBL. 17 REF.Article

LY AURIGAE, NY CEPHEI, AND THE MASS-LUMINOSITY ANOMALY WITHIN O TYPE BINARIESPOPPER DM.1982; ASTROPHYSICAL JOURNAL; ISSN 0004-637X; USA; DA. 1982; VOL. 262; NO 2; PART 1; PP. 641-649; BIBL. 2 P.Article

DISTANCES TO ECLIPSING BINARIES. III: MASSES, RADII, AND ABSOLUTE MAGNITUDES OF 96 STARSLACY CH.1979; ASTROPHYS. J.; USA; DA. 1979; VOL. 228; NO 3 PART. 1; PP. 817-827; BIBL. 2 P.Article

A re-examination of mass-luminosity relations from binary-star dataGRIFFITHS, S. C; HICKS, R. B; MILONE, E. F et al.Journal of the Royal Astronomical Society of Canada. 1988, Vol 82, Num 1, pp 1-12, issn 0035-872XArticle

Mass-Luminosity Relation and Pulsational Properties of Wolf-Rayet StarsFADEYEV, Yu. A.Astronomy letters (Print). 2008, Vol 34, Num 11, pp 772-784, issn 1063-7737, 13 p.Article

The luminosity-core mass relation: why and howTUCHMAN, Y; GLASNER, A; BARKAT, Z et al.The Astrophysical journal. 1983, Vol 268, Num 1, pp 356-360, issn 0004-637XArticle

LUMINOSITIES AND MASSES FOR THREE CENTRAL STARS OF PLANETARY NEBULAE IN THE MAGELLANIC CLOUDS FROM ULTRAVIOLET SPECTROSCOPY WITH THE IUESTECHER TP; MARAN SP; GULL TR et al.1982; ASTROPHYSICAL JOURNAL; ISSN 0004-637X; USA; DA. 1982; VOL. 262; NO 2; PART. 2; PP. L41-L46; H.T. 1; BIBL. 36 REF.Article

THE BRIGHTEST STARS. I: THE UPPER BOUNDARIES OF THE HERTZSPRUNG-RUSSELL DIAGRAMDE JAGER C.1980; GEOPHYS. ASTROPHYS. MONOGR.; NLD; DA. 1980; VOL. 19; PP. 1-17Article

New opacities and first overtone mode CepheidsANTONELLO, E.Astrophysics and space science. 1993, Vol 210, Num 1-2, pp 331-332, issn 0004-640XConference Paper

Pente de la fonction masse pour des étoiles de faible masseMALKOV, O. YU.Astrofizika. 1987, Vol 26, Num 3, pp 477-487, issn 0571-7132Article

The Wolf-Rayet mass-luminosity relationBEECH, M.Astrophysics and space science. 1987, Vol 139, Num 1, pp 149-153, issn 0004-640XArticle

Resonance effects in fundamental, first overtone and double-mode CepheidsANTONELLO, E.Astronomy and astrophysics (Berlin. Print). 1994, Vol 282, Num 3, pp 835-842, issn 0004-6361Article

Mass-luminosity relation and initial mass function at the faint end of the main sequence. Is there a real deficit of very low mass stars?D'ANTONA, F; MAZZITELLI, I.Astronomy and astrophysics (Berlin. Print). 1983, Vol 127, Num 1, pp 149-152, issn 0004-6361Article