EVOLUTION D'UNE ETOILE 16M DE LA SEQUENCE PRINCIPALE A LA PHASE SUPERGEANTE ROUGEVARSHAVSKIJ VI.1972; ASTR. ZH.; S.S.S.R.; DA. 1972; VOL. 49; NO 5; PP. 1055-1058; BIBL. 9 REF.Serial Issue

STRUCTURE DES ENVELOPPES DES SUPERGEANTES ROUGESUUS U.1972; ASTR. SOVET AKAD. NAUK S.S.S.R., NAUCH. INFORM.; S.S.S.R.; DA. 1972; NO 21; PP. 46-50; ABS. ANGL.; BIBL. 4 REF.Serial Issue

ETAT D'EVOLUTION DES SUPERGEANTES BLEUES ET ROUGESFRANTSMAN YU.1976; ISSLEDOV. SOLNCA KRASN. ZVEZD, LATV. S.S.R.; S.S.S.R.; DA. 1976; NO 4; PP. 60-74; ABS. LIT. ANGL.; BIBL. 3 P.Article

RED SUPERGIANTS AND NEUTRINO EMISSION. IISTOTHERS R.1972; ASTROPHYS. J.; U.S.A.; DA. 1972; VOL. 175; NO 3, PART 1; PP. 717-730; BIBL. 2P.Serial Issue

MODEL FOR THE CIRCUMSTELLAR GAS AROUND ALPHA ORIONISJURA M; MORRIS M.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 251; NO 1; PART. 1; PP. 181-189; BIBL. 45 REF.Article

REFLECTION NEBULAE AROUND RED SUPERGIANTS.JURA M; JACOBY G.1976; ASTROPHYS. LETTERS; U.S.A.; DA. 1976; VOL. 18; NO 1; PP. 5-6; BIBL. 15 REF.Article

VARIATIONS DE LA COMPOSITION CHIMIQUE DE L'ENVELOPPE D'UNE SUPERGEANTE ROUGE DE MASSE 5M1972; ASTR. SOVET AKAD. NAUK S.S.S.R., NAUCH. INFORM.; S.S.S.R.; DA. 1972; NO 23; PP. 85-96; ABS. ANGL.; BIBL. 11REF.Serial Issue

A LUMINOSITY DISCRIMINANT FOR RED GIANTS AND SUPERGIANTSSHARPLESS S; WAWRUKIEWICZ AS.1973; ASTR. J.; U.S.A.; DA. 1973; VOL. 78; NO 6; PP. 477-481; BIBL. 16REF.Serial Issue

ABUNDANCE CHANGES IN THE ENVELOPES OF MODERATE MASS STARS AT LATE STAGES OF EVOLUTIONUUS U.sdIN: STELLAR AGES. PROC. I.A.U. COLLOQ. NO.17: MEUDON; 1972; PARIS; IMPR. OBS.; DA. S.D.; PP. XIII.1-XIII.4; BIBL. 6 REF.Conference Paper

THE NUMBERS OF RED SUPERGIANTS AND WR STARS IN GALAXIES: AN EXTREMELY SENSITIVE INDICATOR OF CHEMICAL COMPOSITIONMAEDER A; LEQUEUX J; AZZOPARDI M et al.1980; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1980; VOL. 90; NO 1-2; PP. L17-L20; BIBL. 20 REF.Article

SPORADIC MASS EJECTION IN RED SUPERGIANTSKAFATOS M; MICHALITSIANOS AG.1979; ASTROPHYS. J.; USA; DA. 1979; VOL. 228; NO 3 PART. 2; PP. L115-L118; BIBL. 21 REF.Article

SEQUENCES DE MODELES D'EQUILIBRE POUR LES ETOILES AVEC COMBUSTION D'HELIUM DANS LA REGION DES SUPERGEANTES BLEUES. IIFRANTSMAN YU L; POPOVA EI; DZHULKOVSKIJ YA et al.1974; ASTR. SOVET AKAD. NAUK S.S.S.R., NAUCH. INFORM.; S.S.S.R.; DA. 1974; NO 31; PP. 27-39; ABS. ANGL.; BIBL. 14 REF.Article

DUST FORMATION PROCESSES AROUND RED GIANTS AND SUPERGIANTSDRAINE BT.1981; ASTROPHYS. SPACE SCI. LIBR.; ISSN 0067-0057; NLD; DA. 1981; VOL. 88; PP. 317-333; BIBL. 2 P.Conference Paper

THE LUMINOSITIES OF RED SUPERGIANT VARIABLES IN THE SMALL MAGELLANIC CLOUDCATCHPOLE RM; FEAST MW.1981; MON. NOT. R. ASTRON. SOC.; ISSN 0035-8711; GBR; DA. 1981; VOL. 197; NO 2; PP. 385-391; BIBL. 16 REF.Article

ETUDE DES GROUPEMENTS STELLAIRES DANS LA GALAXIE D'ANDROMIDEEFREMOV YU N.1982; PIS'MA V ASTRONOMICESKIJ ZURNAL; ISSN 507806; SUN; DA. 1982; VOL. 8; NO 10; PP. 585-592; ABS. ENG; BIBL. 16 REF.Article

ATMOSPHERES OF RED SUPERGIANT STARS. II. THE M₂ SUPERGIANT STAR BETELGEUSE.TSUJI T.1976; PUBL. AST. SOC. JAP.; JAP.; DA. 1976; VOL. 28; NO 4; PP. 567-586; BIBL. 1 P.Article

MODEL STUDY OF THE SPHERICITY EFFECTS IN EXTENDED ATMOSPHERES OF LATE-TYPE STARS.WATANABE T; KODAIRA K.1978; PUBL. ASTR. SOC. JAP.; JAP.; DA. 1978; VOL. 30; NO 1; PP. 21-38; BIBL. 1 P. 1/2Article

Périodes, amplitudes et luminosités de supergéantes rougesABRAMYAN, G. V.Astrofizika. 1984, Vol 20, Num 2, pp 239-243, issn 0571-7132Article

Red supergiants in the disk of M81 : Tracing the spatial distribution of star formation 25 myr in the pastDAVIDGE, T. J.Publications of the Astronomical Society of the Pacific. 2006, Vol 118, Num 850, pp 1626-1638, issn 0004-6280, 13 p.Article

The groups of stars with common space motion in the Galaxy. The groups of red supergiants of the luminosity classes I and IIPAVLOVSKAYA, E. D; FILIPPOVA, A. A.Astronomičeskij žurnal. 1990, Vol 67, Num 4, pp 714-722, issn 0004-6299, 9 p.Article

Multiwavelength images of α OrionisCHRISTOU, J. C; HEBDEN, J. C; HEGE, E. K et al.The Astrophysical journal. 1988, Vol 327, Num 2, pp 894-904, issn 0004-637X, 1Article

Nature binaire possible de supernovae particulières de type I: si la supergéante rouge est composante secondaire?CHUGAJ, N. N.Astronomičeskij žurnal. 1986, Vol 63, Num 5, pp 951-957, issn 0004-6299Article

Light curves of the unique M 31 red supergiantSHAROV, A.Pis′ma v Astronomičeskij žurnal. 1993, Vol 19, Num 2, pp 83-86, issn 0320-0108Article

Stratification of optical emission from NGC 6888 as a trace of the interaction between Wolf-Rayet stellar wind and the shell of a red supergiantBYCHKOV, K. V; SITNIK, T. G.Astronomy letters (Print). 2006, Vol 32, Num 6, pp 406-412, issn 1063-7737, 7 p.Article

Are the red supergiants ε Peg and 12 Pup victims of mild s-processing?SMITH, V. V; LAMBERT, D. L.Monthly Notices of the Royal Astronomical Society. 1987, Vol 226, Num 3, pp 563-579, issn 0035-8711Article