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kw.\*:("ETOILE P CYGNI")

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CHANGEMENT OBSERVE DANS LE SPECTRE DE L'ETOILE SYMBIOTIQUE CI CYGNI.GRAVINA R.1975; C.R. ACAD. SCI., B; FR.; DA. 1975; VOL. 280; NO 5; PP. 115-116; H.T. 1; ABS. ANGL.; BIBL. 4 REF.Article

PERTE DE MASSE DANS LES ETOILES.VIGROUX L.1977; RECHERCHE; FR.; DA. 1977; NO 77; PP. 368-369Article

VARIATIONS DES VITESSES RADIALES DE P CYGNILUUD L; GOLLANDSKY O; YARYGINA T et al.1975; PUBL. TARTU. ASTROFIZ. OBS. V. STRUVE, E.S.S.R.; ESTON. S.S.R.; DA. 1975; VOL. 43; PP. 250-255; ABS. ANGL.; BIBL. 4 REF.Article

THE CONTINUOUS SPECTRUM OF P CYGNI IN 1971-1974.HAENNI U; LUUD L.1975; PUBL. TARTU. ASTROFIZ. OBS. V. STRUVE, E.S.S.R.; ESTON. S.S.R.; DA. 1975; VOL. 43; PP. 31-37; ABS. RUSSE; BIBL. 6 REF.Article

THE PROFILE OF HE I LAMBDA 5876 IN THE P-CYGNI-TYPE OF STAR HD 152408.WALBORN NR.1975; PUBL. ASTR. SOC. PACIF.; U.S.A.; DA. 1975; VOL. 87; NO 519; PP. 735-736; BIBL. 8 REF.Article

SOME RELATIONS BETWEEN WOLF-RAYET AND P-CYGNI-TYPE STARSDE GROOT M.1973; INTERNATION. ASTR. UN., SYMP.; NETHERL.; DA. 1973; NO 49; PP. 108-125; BIBL. 1P.; (WOLF-RAYET HIGH TEMP. STARS. PROC. SYMP. NO. 49: BUENOS AIRES; 1971)Conference Paper

P CYGNI PROFILES IN ZETA OPHIUCHI AND ZETA PUPPIS.MORTON DC.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 203; NO 2 PART. 1; PP. 386-398; BIBL. 61 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

TRANSFER OF RESONANCE-LINE RADIATION IN DIFFERENTIALLY EXPANDING ATMOSPHERES. III. FORMATION OF P CYGNI-TYPE LINES BY A DOUBLET LINE OR TWO PARTIALLY "BLENDED" LINES.HEWITT RG; NOERDLINGER PD.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 188; NO 2 PART. 1; PP. 315-326; BIBL. 23 REF.Article

SPECTRA AND FABRY-PEROT INTERFEROMETRY OF AG CARINAE AND THE NEBULA.JOHNSON HM.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 206; NO 2 PART. 1; PP. 469-473; H.T. 1; BIBL. 28 REF.Article

THE VISIBLE AND NEAR INFRARED SPECTRUM OF THE HETEROGENEOUS ATMOSPHERE OF THE B(E) STAR WITH INFRARED EXCESS HD 51585.KLUTZ M; SWINGS JP.1977; ASTR. AND ASTROPHYS.; GERM.; DA. 1977; VOL. 56; NO 1-2; PP. 143-149; BIBL. 20 REF.Article

LONG-TERM CHANGES IN ULTRAVIOLET P CYGNI PROFILES OBSERVED WITH COPERNICUS.SNOW TP JR.1977; ASTROPHYS. J.; U.S.A.; DA. 1977; VOL. 217; NO 3 PART. 1; PP. 760-770; BIBL. 27 REF.Article

ON THE RELATIONSHIPS BETWEEN OF AND WR STARS.CONTI PS.1976; MEM. SOC. R. SCI. LIEGE, 8O; BELG.; DA. 1976; VOL. 9; PP. 193-214; BIBL. 2 P.; (ASTROPHYS. SPECTROSC. COLLOQ. INT. ASTROPHYS. 20; LIEGE; 1975)Conference Paper

A MODEL FOR P CYGNI BASED ON THE HE I SPECTRUM.OEGERLE WR; VAN BLERKOM D.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 208; NO 2 PART. 1; PP. 453-457; BIBL. 9 REF.Article

MASS EJECTION FROM THE O4F STAR ZETA PUPPIS.LAMERS HJGLM; MORTON DC.1976; ASTROPHYS. J., SUPPL. SER.; U.S.A.; DA. 1976; VOL. 32; NO 4; PP. 715-736; BIBL. 1 P.Article

HOURLY VARIATIONS IN OVI P CYGNI PROFILES OF HOT STARS.YORK DG; VIDAL MADJAR A; LAURENT C et al.1977; ASTROPHYS. J.; U.S.A.; DA. 1977; VOL. 213; NO 2 PART. 2; PP. L61-L65; BIBL. 18 REF.Article

AN INFALL MODEL FOR THE T TAURI PHENOMENON.ULRICH RK.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 210; NO 2 PART. 1; PP. 377-391; BIBL. 26 REF.Article

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