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A NOTE ON STELLAR WINDS AND BREEZES1972; PROC. R. SOC. LONDON, A; G.B.; DA. 1972; VOL. 329; NO 1577; PP. 241-249; H.T. 12; BIBL. 4REF.Serial Issue

RADIATIVELY ACCELERATED NOVA ENVELOPESFERLAND GJ; YOUNGER JW.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 2511; NO 1; PART. 2; PP. L17-L20; BIBL. 26 REF.Article

MASS AND ANGULAR MOMENTUM EFFLUXES OF STELLAR WINDS.TYAN YEH.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 206; NO 3 PART. 1; PP. 768-776; BIBL. 10 REF.Article

STELLAR WINDS AND RELATED PHENOMENA IN SURROUNDING NEBULAE.PIKEL'NER SB.1973; COMMENTS ASTROPHYS. SPACE PHYS.; U.S.A.; DA. 1973; VOL. 5; NO 6; PP. 151-158; BIBL. 30 REF.Article

ON THE THEORY OF THERMALLY SUSTAINED STELLAR WINDSSOUFFRIN P.1982; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1982; VOL. 106; NO 1; PP. 14-15; BIBL. 7 REF.Article

DYNAMICS OF IONIZED REGIONSDYSON JE.1978; J. PHYS., COLLOQ.; FRA; DA. 1978; VOL. 39; NO 1; PP. 161-163; ABS. ENG; (MILIEU INTERSTELLAIRE. CONGR. SOC. FR. PHYS.; POITIERS; 1977)Conference Paper

PHOTOSPHERIC FLOW AND STELLAR WINDSPARKER EN.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 251; NO 1; PART. 1; PP. 266-270; BIBL. 26 REF.Article

MAGNETIC BRAKING BY A STELLAR WIND. V. APPROXIMATE DETERMINATION OF THE POLOIDAL FIELD.OKAMOTO I.1975; MONTH. NOT. R. ASTR. SOC.; G.B.; DA. 1975; VOL. 173; NO 2; PP. 357-379; BIBL. 13 REF.Article

RADIATIVE TRANSFER IN EXPANDING ATMOSPHERES.MIHALAS D.1976; IN: PHYS. MOUVEMENTS ATMOS. STELLAIRES. COLLOQ. INT. C.N.R.S.; NICE; 1975; PARIS; C.N.R.S.; DA. 1976; PP. 347-418 ( 21P.); ABS. FR.; BIBL. 1 P. 1/2Conference Paper

STELLAR MASS LOSS.LUCY LB.1975; MEM. SOC. R. SCI. LIEGE, 8.; BELG.; DA. 1975; VOL. 8; PP. 359-367 (8P.); BIBL. 25 REF.; (PROBL. HYDRODYN. STELLAIRE. 19E. COLLOQ. INT. ASTROPHYS.; LIEGE; 1974)Conference Paper

THE INFLUENCE OF ROTATION AND STELLAR WINDS UPON THE BE PHENOMENON.MASSA D.1975; PUBL. ASTR. SOC. PACIF.; U.S.A.; DA. 1975; VOL. 87; NO 519; PP. 777-784; BIBL. 35 REF.Article

MODELING OF STEADY, ROTATIONAL, TRANSONIC WINDS FROM ROTATING STARS AND GALAXIESKOPRIVA DA; JOKIPH JR.1983; ASTROPHYSICAL JOURNAL; ISSN 0004-637X; USA; DA. 1983; VOL. 267; NO 1; PART. 1; PP. 62-79; BIBL. 37 REF.Article

THE EXTENSION OF OB STAR WINDS TO LOWER LUMINOSITIESSNOW TP JR.1982; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1982; VOL. 253; NO 1; PART. 2; PP. 39-42; BIBL. 7 REF.Article

PROPERTIES OF OPTICALLY THICK WINDS DRIVEN BY RADIATION PRESSUREFRIEDJUNG M.1981; ASTROPHYS. SPACE SCI. LIBR.; ISSN 0067-0057; NLD; DA. 1981; VOL. 89; PP. 495-497; BIBL. 8 REF.Conference Paper

RADIO RECOMBINATION LINES IN MWC 349ALTENHOFF WJ; STRITTMATTER PA; WENDKER HJ et al.1981; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1981; VOL. 93; NO 1-2; PP. 48-52; BIBL. 24 REF.Article

THE STRUCTURE OF OPTICALLY THICK WINDS IN CLASSICAL NOVAERUGGLES CLN; BATH GT.1979; ASTR. AND ASTROPHYS.; DEU; DA. 1979; VOL. 80; NO 1; PP. 97-103; BIBL. 29 REF.Article

NOVA CYGNI 1975: WIND AND VARIATIONS.FABIAN AC; PRINGLE JE.1977; MONTH. NOT. R. ASTR. SOC.; G.B.; DA. 1977; VOL. 180; NO 3; PP. 749-754; BIBL. 11 REF.Article

RADIATION-DRIVEN STELLAR WINDS.CASTOR JI; ABBOTT DC; KLEIN RI et al.1976; IN: PHYS. MOUVEMENTS ATMOS. STELLAIRES. COLLOQ. INT. C.N.R.S.; NICE; 1975; PARIS; C.N.R.S.; DA. 1976; PP. 363-418 (37P.); ABS. FR.; BIBL. 1 P. 1/2Conference Paper

STELLAR WINDS AND ACCRETION IN MASSIVE X-RAY BINARIES.LAMERS HJGLM; VAN DEN HEUVEL EPJ; PETTERSON JA et al.1976; ASTR. AND ASTROPHYS.; GERM.; DA. 1976; VOL. 49; NO 3; PP. 327-335; BIBL. 63 REF.Article

POLYTROPIC SUBSONIC STELLAR WINDS WITH MAGNETIC FIELDSDURNEY B.1972; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1972; VOL. 17; NO 2; PP. 489-498; BIBL. 17REF.Serial Issue

AN ESTIMATE OF STELLAR WIND MASS LOSS DURING THE RED GIANT PHASE OF EVOLUTIONHEASLEY JN JR; MENGEL JG.1972; OBSERVATORY; G.B.; DA. 1972; VOL. 92; NO 988; PP. 93-96; BIBL. 27REF.Serial Issue

MASS LOSS FROM CENTRAL STARS OF PLANETARY NEBULAEPERINOTTO M.1983; SYMPOSIUM - INTERNATIONAL ASTRONOMICAL UNION; ISSN 0074-1809; NLD; DA. 1983; NO 103; PP. 323-335; BIBL. 2 P.Conference Paper

THE RATIO OF DEUTERIUM TO HYDROGEN IN INTERSTELLAR SPACE. THE LINE OF SIGHT TO EPSILON PERSEIVIDAL MADJAR A; LAURENT C; GRY C et al.1983; ASTRONOMY AND ASTROPHYSICS; ISSN 0004-6361; DEU; DA. 1983; VOL. 120; NO 1; PP. 58-62; BIBL. 42 REF.Article

WIND ACCELERATION IN EARLY-TYPE STARS: THE MOMENTUM PROBLEM AND THE TERMINAL VELOCITYPANAGIA N; MACCHETTO F.1982; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1982; VOL. 106; NO 2; PP. 266-273; BIBL. 22 REF.Article

ON STELLAR WIND ACCRETION IN WIDELY SEPARATED X-RAY BINARIES, AND THE NATURE OF 4U 0115+63AVNI Y; GOLDMAN I.1981; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1981; VOL. 102; NO 1; PP. 12-16; BIBL. 27 REF.Article

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