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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

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

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

ON THE ANGULAR MOMENTUM OF STARS AND THE MAIN SEQUENCE STELLAR MODELSVIRGOPIA N.1972; MEM. SOC. ASTR. ITAL.; ITAL.; DA. 1972; VOL. 43; NO 4; PP. 813-821; ABS. ITAL.; BIBL. 21REF.Serial Issue

RADII OF SINGLE MAIN SEQUENCE STARS (AOV-G2V): COMPARISON WITH RADII DETERMINED USING BINARY SYSTEMSSHALLIS MJ; BLACKWELL DE.1980; ASTR. AND ASTROPHYS.; DEU; DA. 1980; VOL. 81; NO 3; PP. 336-339; BIBL. 24 REF.Article

CONVECTIVE OVERSHOOTING IN MAIN-SEQUENCE MODELSCOGAN BC.1975; ASTROPHYS. J.; USA; DA. 1975; VOL. 201; NO 3 PART. 1; PP. 637-640; BIBL. 3 REF.Article

PHOTOMETRIC SCANS OF HALPHA IN EARLY A-STARS.FRANDSEN S.1975; ASTR. AND ASTROPHYS.; GERM.; DA. 1975; VOL. 43; NO 2; PP. 267-273; BIBL. 18 REF.Article

THE INFLUENCE OF THE OPACITY VALUES AND MINING LENGTH ON THE EVOLUTION OF POPULATION II MAIN SEQUENCE STARS.STABELL R.1975; ASTR. AND ASTROPHYS.; GERM.; DA. 1975; VOL. 44; NO 2; PP. 315-319; BIBL. 12 REF.Article

VIBRATIONAL INSTABILITY OF A 1 M CERCLE.STAR TOWARDS NON-RADIAL OSCILLATIONS.BOURY A; GABRIEL M; NOELS A et al.1975; ASTR. AND ASTROPHYS.; GERM.; DA. 1975; VOL. 41; NO 3-4; PP. 279-285; BIBL. 22 REF.Article

THE MAIN SEQUENCE STARS AND THE PHOTON-NEUTRINO COUPLING THEORY OF WEAK INTERACTIONS.NISHIDA M; YAMASAKI A.1974; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1974; VOL. 30; NO 1; PP. 225-231; BIBL. 28 REF.Article

CALCULATION OF THEORETICAL ROTATIONAL LINE PROFILES FOR THE DETERMINATION OF V SIN I IN THE SPECTRAL RANGE O9-F8.COLLINS GW II.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 191; NO 1 PART. 1; PP. 157-164; BIBL. 22 REF.Article

ON STELLAR STRUCTURE IN NON-UNIFORM ROTATION. III. NON-BAROTROPIC MODELS IN FAST ROTATIONTUOMINEN IV.1972; ANN. ACAD. SCI. FENN., A6; FINL.; DA. 1972; NO 393; PP. 1-20; BIBL. 9 REF.Serial Issue

THE MAIN SEQUENCE DEFINED BY TRIGONOMETRICAL PARALLAXES.WOOLLEY R.1976; MONTH. NOT. R. ASTR. SOC.; G.B.; DA. 1976; VOL. 174; NO 3; PP. 621-626; BIBL. 10 REF.Article

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