NUMERICAL IMPLEMENTATION OF A PERTURBATION-THEORY UP TO 3RD ORDER FOR ROTATING POLYTROPIC STARS - STRUCTURE PARAMETERS UNDER DIFFERENTIAL ROTATION

被引：7

作者：

GEROYANNIS, VS ^{[1
]}

VALVI, FN ^{[1
]}

机构：

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

来源：

ASTROPHYSICAL JOURNAL | 1987年 / 312卷 / 01期

关键词：

D O I：

10.1086/164864

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：219 / 226

页数：8

共 17 条

[1]

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[5]

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VALVI, FN .

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[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 .

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

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TOKIS, JN ;

VALVI, FN .

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[10] LEVEL SURFACE APPROACH FOR UNIFORMLY ROTATING, AXISYMMETRIC POLYTROPES [J].

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ASTROPHYSICAL JOURNAL, 1983, 269 (01) :303-308

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