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Results 1 to 25 of 1409

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LINE STRENGTHS FOR YELLOW SUPERGIANTS AND CEPHEIDS.SCHMIDT EG; ROSENDHAL JD; JEWSBURY CP et al.1974; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1974; VOL. 29; NO 2; PP. 397-414; BIBL. 7 REF.Article

COULEURS INTRINSEQUES DES CEPHEIDES CLASSIQUES ET DES SUPERGEANTES JAUNES1972; ASTR. CIRK., IZDAV. BJURO ASTR. SOOBSHCH. AKAD. NAUK S.S.S.R.; S.S.S.R.; DA. 1972; NO 679; PP. 5-7; BIBL. 6REF.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

PARAMETRES CINEMATIQUES DES SUPERGEANTES B)KARIMOVA DK; PAVLOVSKAYA ED.1976; ASTR. ZH.; S.S.S.R.; DA. 1976; VOL. 53; NO 3; PP. 495-500; ABS. ANGL.; BIBL. 10 REF.Article

A COMPARISON OF GALACTIC AND LARGE MAGELLANIC CLOUD G. TYPE SUPERGIANTS BY A METHOD OF SPECTRUM SYNTHESIS.FRY MA; ALLER LH.1975; ASTROPHYS. J., SUPPL. SER.; U.S.A.; DA. 1975; VOL. 29; NO 275; PP. 55-75; BIBL. 87 REF.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

SPECTROSCOPIC AND PHOTOMETRIC OBSERVATIONS OF M SUPERGIANTS IN CARINAHUMPHREYS RM; STRECKER DW; NEY EP et al.1972; ASTROPHYS. J.; U.S.A.; DA. 1972; VOL. 172; NO 1, PART 1; PP. 75-88; BIBL. 25REF.Serial Issue

THE LUMINOSITY DEPENDENCE OF THE 1.65 N FLUX FROM K AND EARLY M STARS. OBSERVATIONS AND INTERPRETATION.BELL RA; GUSTAFSSON B; NORDH HL et al.1976; ASTR. AND ASTROPHYS.; GERM.; DA. 1976; VOL. 46; NO 3; PP. 391-396; BIBL. 18 REF.Article

THE OPEN CLUSTER NGC 7419 AND ITS M7 SUPERGIANT IRC+60375.FAWLEY WM; COHEN M.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 193; NO 2 PART. 1; PP. 367-372; BIBL. 32 REF.Article

1612-MHZ SURVEY OF M SUPERGIANTS.BOWERS PF.1975; ASTR. J.; U.S.A.; DA. 1975; VOL. 80; NO 7; PP. 512-514; BIBL. 7 REF.Article

STELLAR WINDS FROM HOT SUPERGIANTS.HUTCHINGS JB.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 203; NO 2 PART. 1; PP. 438-447; BIBL. 34 REF.Article

A-TYPE SUPERGIANTS: A LIST OF LINE INTENSITIES AND RADIAL VELOCITY MEASUREMENTSAYDIN C.1972; ASTR. AND ASTROPHYS., SUPPL. SER.; GERM.; DA. 1972; VOL. 7; NO 3; PP. 331-354; BIBL. 11REF.Serial Issue

A SEARCH FOR SPECTRUM VARIABILITY IN HD 14688 AND ZETA 1 SCORPII.WALBORN NR.1975; PUBL. ASTR. SOC. PACIF.; U.S.A.; DA. 1975; VOL. 87; NO 519; PP. 759-761; BIBL. 6 REF.Article

THEORETICAL COLOURS FORM F AND G SUPERGIANTS.BELL RA; PARSONS SB.1974; MONTH. NOT. R. ASTR. SOC.; G.B.; DA. 1974; VOL. 169; NO 1; PP. 71-78; BIBL. 23 REF.Article

A NITROGEN B SUPERGIANT IN A PECULAR ECLIPSING SYSTEMWALBORN NR.1972; ASTROPHYS. J.; U.S.A.; DA. 1972; VOL. 176; NO 3 PART 2; PP. 119-121; BIBL. 16REF.Serial Issue

ASTRONOMICAL INFRARED SPECTROSCOPY WITH A CONNES-TYPE INTERFEROMETER. III.ALPHA ORIONIS, 2600-3450CM-1BEER R; HUTCHINSON RB; NORTON RH et al.1972; ASTROPHYS. J.; U.S.A.; DA. 1972; VOL. 172; NO 1, PART 1; PP. 89-115; BIBL. 35REF.Serial Issue

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

PROFONDEUR DU PETIT NUAGE DE MAGELLAN RELEVEE PAR LES SUPERGEANTES BLEUESAZZOPARDI M.1982; STRUCTURE DU PETIT NUAGE DE MAGELLAN. JOURNEES DE STRASBOURG. REUNION. 4/1982-02-23/STRASBOURG; FRA; STRASBOURG: OBSERVATOIRE DE STRASBOURG; DA. 1982; PP. 20-37; BIBL. 3 P.Conference Paper

NOTE ON THE SPECTRA OF SOME BRIGHT A-TYPE SUPERGIANTS IN THE LARGE MAGELLANIC CLOUD.FEHRENBACH C; JASCHEK M; JASCHEK C et al.1977; ASTR. AND ASTROPHYS.; GERM.; DA. 1977; VOL. 54; NO 2; PP. 367-368; BIBL. 7 REF.Article

A CATALOGUE OF A- AND F-TYPE SUPERGIANTS IN THE LARGE MAGELLANIC CLOUD.STOCK J; OSBORN W; IBANEZ M et al.1976; ASTR. AND ASTROPHYS., SUPPL. SER.; GERM.; DA. 1976; VOL. 24; NO 1; PP. 35-52; BIBL. 21 REF.Article

THE 12C/13C RATIO IN STELLAR ATMOSPHERES. II. CN AND CO IN ALPHA ORIONIS.LAMBERT DL; DEARBORN DS; SNEDEN C et al.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 193; NO 3 PART. 1; PP. 621-630; BIBL. 23 REF.Article

AGE AND INITIAL CHEMICAL COMPOSITION OF SUPERGIANT STARS AS FUNCTION OF DISTANCE FROM THE GALACTIC CENTERBARBARO G; CHIOSI C.sdIN: STELLAR AGES. PROC. I.A.U. COLLOQ. NO 17; MEUDON; 1972; PARIS; IMPR. OBS.; DA. S.D.; PP. XV.1-XV.15; BIBL. 15 REF.Conference Paper

THE CIRCUMSTELLAR SHELLS AND MASS LOSS RATES OF FOUR M SUPERGIANTS.BERNAT AP.1977; ASTROPHYS. J.; U.S.A.; DA. 1977; VOL. 213; NO 3, PART. 1; PP. 756-766; BIBL. 38 REF.Article

THE MASS LOSS FROM THE 09.5 IB SUPERGIANT, ZETA ORIONIS DERIVED FROM HALPHA PROFILE.HEARN AG.1975; ASTR. AND ASTROPHYS.; GERM.; DA. 1975; VOL. 40; NO 3; PP. 277-283; BIBL. 19 REF.Article

THE SPECTRUM OF THE SUPERGIANT EPSILON ORIONIS (B0IA). I. IDENTIFICATIONS, EQUIVALENT-WIDTHS, LINE PROFILES1972; ASTR. AND ASTROPHYS., SUPPL. SER.; GERM.; DA. 1972; VOL. 7; NO 1; PP. 113-132; BIBL. 18REF.Serial Issue

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