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SOME PHOTOMETRIC CHARACTERISTICS OF YOUNG STARS.MENDOZA EEV.1975; PUBL. ASTR. SOC. PACIF.; U.S.A.; DA. 1975; VOL. 87; NO 518; PP. 495-497; BIBL. 8 REF.Article

NON-LINEAR PULSATIONS OF UPPER MAIN SEQUENCE STARS. I. A PERTURBATION APPROACH1973; MONTH. NOT. R. ASTR. SOC.; G.B.; DA. 1973; VOL. 162; NO 2; PP. 143-168; BIBL. 22REF.Serial Issue

ON THE METALLICITY OF THE MAIN SEQUENCE STARS IN M67MORGAN WW; ABT HA.1973; ASTR. J.; U.S.A.; DA. 1973; VOL. 78; NO 5; PP. 386-388; BIBL. 6 REF.Serial Issue

CONTRIBUTION AUX ETUDES DE MODELES D'ETOILES DE LA SEQUENCE PRINCIPALEANGELOV T.1975; PUBL. OBS. ASTR. BEOGRAD; YOUGOSL.; DA. 1975; NO 20; PP. 110-122; ABS. ANGL.; BIBL. 7 REF.; (ZB. RAD. NAC. KONF. JUGOSL. ASTRON.; BEOGRAD; 1973)Conference Paper

TENTATIVE IDENTIFICATION OF MAIN-SEQUENCE STARS IN THE NUCLEAR BULGE OF THE GALAXY.VAN DEN BERGH S.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 188; NO 1 PART. 2; PP. 9-10; BIBL. 13 REF.Article

CONVECTIVE OVERSHOOTING IN MAIN SEQUENCE MODELS.COGAN BC.1975; ASTR. SOC. AUSTRAL., PROC.; AUSTRAL.; DA. 1975; VOL. 2; NO 6; PP. 355-356; BIBL. 3 REF.; (ASTRON. SOC. AUSTRALIA. ANN. GEN. MEET. 9 PROC.; PARKES; 1975)Conference Paper

A COMPARISON OF HOMOGENEOUS STELLAR MODELS BASED ON THE COX-STEWART AND CARSON OPACITIES.STOTHERS R.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 194; NO 3 PART. 1; PP. 695-697; BIBL. 20 REF.Article

THE STRUCTURE OF CHEMICALLY HOMOGENEOUS MAIN-SEQUENCE STARSMOTZ L.1972; PUBL. ASTR. SOC. PACIF.; U.S.A.; DA. 1972; VOL. 84; NO 500; PP. 465-488; BIBL. 33REF.Serial Issue

UNCERTAINTIES IN THE OBSERVABLE PROPERTIES OF LOWER MAIN SEQUENCE STELLAR MODELS1972; MONTH. NOT. R. ASTR. SOC.; G.B.; DA. 1972; VOL. 156; NO 3; PP. 291-296; BIBL. 9REF.Serial Issue

MODELS OF STELLAR DIFFERENTIAL ROTATION ON THE LOWER MAIN SEQUENCEMOSS D; VILHU O.1983; ASTRONOMY AND ASTROPHYSICS; ISSN 0004-6361; DEU; DA. 1983; VOL. 119; NO 1; PP. 47-53; BIBL. 17 REF.Article

RESPONSE OF LOW-MASS MAIN SEQUENCE STARS TO ACCRETIONFUJIMOTO MY; IBEN I JR; BECKER SA et al.1981; ASTROPHYS. SPACE SCI. LIBR.; ISSN 0067-0057; NLD; DA. 1981; VOL. 89; PP. 401-403; BIBL. 5 REF.Conference Paper

STRAINED COORDINATE METHODS IN ROTATING STARS. II. MAIN-SEQUENCE STARS.SMITH BL.1977; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1977; VOL. 47; NO 1; PP. 61-78; BIBL. 24 REF.Article

MEASUREMENTS OF MAGNETIC FIELDS IN YOUNG MAIN-SEQUENCE STARS.BOESGAARD AM.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 188; NO 3 PART. 1; PP. 567-569; BIBL. 19 REF.Article

ON THE MAGNETIC FIELDS OF UPPER MAIN SEQUENCE STARS.MAHESWARAN M.1974; ASTR. AND ASTROPHYS.; GERM.; DA. 1974; VOL. 37; NO 1; PP. 169-178; BIBL. 19 REF.Article

PULSATIONS RADIALES DES ETOILES DELTA SCUTI. I. INSTABILITE VIS-A-VIS DES VIBRATIONS D'UNE ETOILE DE 1,5 M CERCLE. DE LA SEQUENCE PRINCIPALEPAMYATNYKH AA.1974; ASTR. SOVET AKAD. NAUK S.S.S.R., NAUCH. INFORM.; S.S.S.R.; DA. 1974; NO 29; PP. 108-123; BIBL. 18 REF.Article

AN ANALYSIS OF THE PULSATIONAL STABILITY OF VERY LOW MASS STARS ON THE HYDROGEN AND DEUTERIUM MAIN SEQUENCE.OPOIEN JW; GROSSMAN AS.1974; ASTR. AND ASTROPHYS.; GERM.; DA. 1974; VOL. 37; NO 2; PP. 335-338; BIBL. 15 REF.Article

PHOTOMETRIC PARALLAXES OF NEARBY MAIN-SEQUENCE STARS WITH ANNUAL PROPER MOTION OF 0.7'' OR MORE DERIVED FROM EGGEN'S B, V AND R, I DATAGLIESE W.1982; ASTRON. ASTROPHYS., SUPPL. SER.; ISSN 0365-0138; DEU; DA. 1982; VOL. 47; NO 3; PP. 471-480; BIBL. DISSEM.Article

STARS WITH ANOMALOUS MASS: IS THERE FUNNY BUSINESS IN THE MAIN SEQUENCE.WHEELER JC.1979; COMMENTS OU ASTROPHYS.; GBR; DA. 1979; VOL. 8; NO 5; PP. 133-147; BIBL. 44 REF.Article

EFFECTS OF CONVECTIVE OVERSHOOT ON LITHIUM DEPLETION IN MAIN-SEQUENCE STARS.STRAUS JM; BLAKE JB; SCHRAMM DN et al.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 204; NO 2 PART. 1; PP. 481-487; BIBL. 28 REF.Article

NONLINEAR CONVECTIVE MOTION IN SHALLOW CONVECTIVE ENVELOPES.DEUPREE RG.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 205; NO 1 PART. 1; PP. 286-294; BIBL. 21 REF.Article

THE GAP IN THE TWO-COLOR DIAGRAM OF MAIN-SEQUENCE STARS.BOHM VITENSE E; CANTERNA R.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 194; NO 3 PART. 1; PP. 629-635; BIBL. 33 REF.Article

INTRINSIC ULTRAVIOLET COLORS FROM OAO-2 CELESCOPE OBSERVATIONS FOR STARS ON THE MAIN SEQUENCEHARAMUNDANIS K; PAYNE GAPOSCHKIN C.1973; ASTR. J.; U.S.A.; DA. 1973; VOL. 78; NO 5; PP. 395-400; BIBL. 20 REF.Serial Issue

ITERATIVE NONLINEAR PULSATIONS IN MASSIVE STARS. II. TERMS UP TO SECOND ORDERSIMON NR.1972; ASTR. AND ASTROPHYS.; GERM.; DA. 1972; VOL. 21; NO 1; PP. 51-55; BIBL. 17 REF.Serial Issue

AGE CALIBRATIONS FOR POPULATION I COMPOSITIONSHEJLESEN PM; JOERGENSEN HE; PETERSEN JO et al.sdIN: STELLAR AGES. PROC. I.A.U. COLLOQ. NO 17; MEUDON; 1972; PARIS; IMPR. OBS.; DA. S.D.; PP. XVII.1-XVII.36; BIBL. 1 P.Conference Paper

THE CHEMICALLY PECULIAR STARS OF THE UPPER MAIN SEQUENCEPRESTON GW.1973; NUCL. INTRUM. METHODS; NETHERL.; DA. 1973; VOL. 110; PP. 405-410; BIBL. 48 REF.; PROC. 3TH INT. CONF. BEAM-FOIL SPECTROM.; TUCSON, ARIZ.; 1972Conference Paper

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