CHANDRASEKHAR PERTURBATION METHOD-ORIENTED THEORIES UP TO 3RD ORDER FOR UNIFORMLY AND DIFFERENTIALLY-ROTATING POLYTROPIC STARS - ERROR-REMOVING TECHNIQUES

被引：6

作者：

GEROYANNIS, VS ^{[1
]}

VALVI, FN ^{[1
]}

机构：

[1] UNIV PATRAS,DEPT MATH,PATRAS,GREECE

来源：

ASTROPHYSICS AND SPACE SCIENCE | 1986年 / 126卷 / 01期

关键词：

D O I：

10.1007/BF00644180

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：119 / 132

页数：14

共 10 条

[1]

[Anonymous], 2016, MNRAS, DOI DOI 10.1093/MNRAS/STW2088

[2]

CHANDRASEKHAR S, 1962, AP J, V137, P1082

[3]

Chandrasekhar S., 1933, MON NOT R ASTRON SOC, V93, P449, DOI [10.1093/mnras/93.6.449, DOI 10.1093/MNRAS/93.6.449]

[4]

Chandrasekhar S., 1933, MON NOT R ASTRON SOC, V93, P390

[5] NON-RADIAL OSCILLATIONS AND BETA CANIS MAJORIS STARS .2. EFFECT OF DIFFERENTIAL ROTATION [J].

CLEMENT, MJ .

ASTROPHYSICAL JOURNAL, 1967, 150 (2P1) :589-&

[6]

Conte S. D., 1980, ELEMENTARY NUMERICAL

[7] CHANDRASEKHAR PERTURBATION METHOD ORIENTED THEORIES - 3RD-ORDER RESULTS FOR UNIFORMLY AND DIFFERENTIALLY ROTATING POLYTROPIC STARS - RELIABILITY AND ACCURACY OF 1ST-ORDER AND 2ND-ORDER RESULTS FOR UNIFORM ROTATION [J].

GEROYANNIS, VS ;

VALVI, FN .

ASTROPHYSICAL JOURNAL, 1985, 299 (02) :695-705

[8] STRUCTURE-DISTORTION OF POLYTROPIC STARS BY DIFFERENTIAL ROTATION - 3RD-ORDER PERTURBATION-THEORY [J].

GEROYANNIS, VS ;

ANTONAKOPOULOS, GA .

ASTROPHYSICS AND SPACE SCIENCE, 1981, 74 (01) :97-110

[9] 2ND-ORDER PERTURBATION-THEORY FOR DIFFERENTIALLY ROTATING GASEOUS POLYTROPES [J].

GEROYANNIS, VS ;

TOKIS, JN ;

VALVI, FN .

ASTROPHYSICS AND SPACE SCIENCE, 1979, 64 (02) :359-389

[10] SLOWLY ROTATING POLYTROPES [J].

KOVETZ, A .

ASTROPHYSICAL JOURNAL, 1968, 154 (3P1) :999-&

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