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Results 1 to 25 of 42

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ON THE CONDITIONS FOR HOMOGENEOUS STELLAR MODELS TO HAVE ONLY REAL SECULAR EIGENVALUESGABRIEL M; NOELS A.1972; ASTR. AND ASTROPHYS.; GERM.; DA. 1972; VOL. 20; NO 3; PP. 455-459; BIBL. 13REF.Serial Issue

SECULAR STABILITY. IV. THE EFFECTS OF SHELL SOURCES ON THE SECULAR SPECTRUMAIZENMAN ML; PERDANG J.1973; ASTR. AND ASTROPHYS.; GERM.; DA. 1973; VOL. 25; NO 1; PP. 53-57; BIBL. 7REF.Serial Issue

EVOLUTION AND SECULAR STABILITY OF STELLAR MODELS CROSSING THE HERTZSPRUNG GAP FOR M=4, 6 AND 8 M CERCLE..LAUTERBORN D; SIQUIG RA.1976; ASTR. AND ASTROPHYS.; GERM.; DA. 1976; VOL. 49; NO 2; PP. 285-292; BIBL. 30 REF.Article

INFLUENCE OF THE VARIATION OF THE CONVECTIVE ZONE BOUNDARIES ON THE SECULAR STABILITY OF STARS.GABRIEL M; NOELS A.1974; ASTR. AND ASTROPHYS.; GERM.; DA. 1974; VOL. 34; NO 3; PP. 455-456; BIBL. 3 REF.Article

ON USING ENTROPY ARGUMENTS TO STUDY THE EVOLUTION AND SECULAR STABILITY OF SPHERICAL STELLAR-DYNAMICAL SYSTEMS.IPSER JR.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 193; NO 2 PART. 1; PP. 463-470; BIBL. 11 REF.Article

ABUNDANCE PERTURBATIONS, STELLAR EVOLUTION, AND SECULAR STABILITYAIZENMAN ML; PERDANG J.sdIN: STELLAR AGES. PROC. I.A.U. COLLOQ. NO.17: MEUDON; 1972; PARIS; IMPR. OBS.; DA. S.D.; PP. XXXV.1-XXXV.11; BIBL. 8 REF.Conference Paper

ISLAND SOLUTIONS IN LINEAR SERIES OF STATIC STELLAR MODELS WITH CORE HELIUM AND SHELL HYDROGEN BURNING FOR M=5, 7 AND 9 M CERCLE..LAUTERBORN D; SIQUIG RA.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 191; NO 2 PART. 1; PP. 589-592; BIBL. 9 REF.Article

SECULAR STABILITY OF AN 8 M STAR DURING CENTRAL HELIUM BURNINGNOELS A; GABRIEL M.1973; ASTR. AND ASTROPHYS.; GERM.; DA. 1973; VOL. 24; NO 2; PP. 201-208; BIBL. 11REF.Serial Issue

NON-RADIAL SECULAR STABILITY OF THE HYDROGEN BURNING SHELL IN STARS OF 1.1 M CERCLE. AND 8 M CERCLE..GABRIEL M; NOELS A.1976; ASTR. AND ASTROPHYS.; GERM.; DA. 1976; VOL. 46; NO 2; PP. 313-316; BIBL. 7 REF.Article

DISCUSSION OF SIMPLE STABILITY CRITERIA FOR STARS WITH CENTRAL HELIUM BURNING.GABRIEL M; REFSDAL S; RITTER H et al.1975; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1975; VOL. 36; NO 2; PP. 439-450; BIBL. 10 REF.Article

SOME COMMENTS ON SECULAR STABILITY CRITERIA AND APPLICATIONSDEMARET J; LEDOUX P.1973; ASTR. AND ASTROPHYS.; GERM.; DA. 1973; VOL. 23; NO 1; PP. 111-116; BIBL. 25REF.Serial Issue

THE EQUILIBRIUM SERIES AND THE RECULAR STABILITY OF ISOTHERMAL TWO-COMPONENT STAR CLUSTERSYOSHIZAWA M; INAGAKI S; NISHIDA MT et al.1978; PUBL. ASTR. SOC. JAP.; JPN; DA. 1978; VOL. 30; NO 2; PP. 279-294; BIBL. 22 REF.Article

ON THE BUBBLE METHOD OF STABILITY ANALYSIS.SMITH RC; FRICKE KJ.1975; MONTH. NOT. R. ASTR. SOC.; G.B.; DA. 1975; VOL. 172; NO 3; PP. 577-584; BIBL. 7 REF.Article

SECULAR STABILITY. V. THE PERTURBATION OF CHEMICAL ABUNDANCESAZEINMAN ML; PERDANG J.1973; ASTR. AND ASTROPHYS.; GERM.; DA. 1973; VOL. 23; NO 2; PP. 209-214; BIBL. 6 REF.Serial Issue

STATIONARY MOTIONS OF A TRIAXIAL BODY AND THEIR STABILITIESKINOSHITA H.1972; PUBL. ASTR. SOC. JAP.; JAP.; DA. 1972; VOL. 24; NO 3; PP. 409-417; BIBL. 10REF.Serial Issue

THEORETICAL EVOLUTION OF EXTREMELY METAL-POOR STARS.WAGNER RL.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 191; NO 1 PART. 1; PP. 173-182; BIBL. 48 REF.Article

SECULAR STABILITY OF STATIC MODELS DURING CENTRAL HELIUM BURNINGGABRIEL M; NOELS A.1973; ASTR. AND ASTROPHYS.; GERM.; DA. 1973; VOL. 25; NO 2; PP. 313-317; BIBL. 15REF.Serial Issue

INNERMOST PARTS OF ACCRETION DISKS ARE THERMALLY AND RECULARLY STABLEABRAMOWICZ MA.1981; NATURE (LOND.); ISSN 0028-0836; GBR; DA. 1981; VOL. 294; NO 5838; PP. 235-236; BIBL. 3 REF.Article

ON THE SECULAR INSTABILITY FROM THERMAL CONDUCTIVITY IN ROTATING STARSLINDBLOM L.1979; ASTROPHYS. J.; USA; DA. 1979; VOL. 233; NO 3 PART. 1; PP. 974-980; BIBL. 8 REF.Article

ON THE GRAVOTHERMAL CATASTROPHE.NAKADA Y.1978; PUBL. ASTR. SOC. JAP.; JAP.; DA. 1978; VOL. 30; NO 1; PP. 57-66; BIBL. 15 REF.Article

SECULAR STABILITY: APPLICATIONS TO STELLAR STRUCTURE AND EVOLUTIONHANSEN CJ.1978; ANNU. REV. ASTR. ASTROPHYS.; USA; DA. 1978; VOL. 16; PP. 15-32; BIBL. 2 P.Article

STABILITY OF SOLAR SYSTEMKOPAL Z.1980; MOON AND PLANETS; NLD; DA. 1980; VOL. 22; NO 1; PP. 5-11; BIBL. 28 REF.Article

ON SECULAR STABILITY, SECULAR INSTABILITY, AND POINTS OF BIFURCATION OF ROTATING GASEOUS MASSES.HUNTER C.1977; ASTROPHYS. J.; U.S.A.; DA. 1977; VOL. 213; NO 2 PART. 1; PP. 497-517; BIBL. 29 REF.Article

A NEW CRITERION FOR SECULAR INSTABILITY OF RAPIDLY ROTATING STARS.BARDEEN JM; FRIEDMAN JL; SCHUTZ BF et al.1977; ASTROPHYS. J.; U.S.A.; DA. 1977; VOL. 217; NO 1 PART. 2; PP. L49-L53; BIBL. 17 REF.Article

SECULAR STABILITY. VII. AN ANALYTIC MODEL DISPLAYING A CONTINUOUS SPECTRUM.AIZENMAN ML; PERDANG J.1976; ASTR. AND ASTROPHYS.; GERM.; DA. 1976; VOL. 51; NO 2; PP. 263-268; BIBL. 12 REF.Article

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