CHANDRASEKHARS PERTURBATION METHOD ORIENTED THEORIES UP TO 3RD-ORDER - STRUCTURE PARAMETERS FOR ROTATING POLYTROPIC STARS

被引:6
作者
GEROYANNIS, VS [1 ]
VALVI, FN [1 ]
机构
[1] UNIV PATRAS,DEPT MATH,PATRAS,GREECE
关键词
D O I
10.1086/191250
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:139 / 149
页数:11
相关论文
共 11 条
[1]  
[Anonymous], 2016, MNRAS, DOI DOI 10.1093/MNRAS/STW2088
[2]  
Chandrasekhar S., 1933, MON NOT R ASTRON SOC, V93, P449, DOI [10.1093/mnras/93.6.449, DOI 10.1093/MNRAS/93.6.449]
[3]  
Chandrasekhar S., 1933, MON NOT R ASTRON SOC, V93, P390
[4]  
Chandrasekhar S., 1933, MON NOT R ASTRON SOC, V93, P539, DOI [10.1093/mnras/93.8.539a, DOI 10.1093/MNRAS/93.8.539A]
[5]   3RD-ORDER PERTURBATION-THEORY - STRUCTURE PARAMETERS OF UNIFORMLY ROTATING POLYTROPIC STARS AND IMPROVEMENT AND ACCURACY OF THE RESULTS [J].
GEROYANNIS, VS ;
VALVI, FN .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1986, 62 (02) :363-371
[6]   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
[7]   NUMERICAL IMPLEMENTATION OF A PERTURBATION-THEORY UP TO 3RD ORDER FOR ROTATING POLYTROPIC STARS - STRUCTURE PARAMETERS UNDER DIFFERENTIAL ROTATION [J].
GEROYANNIS, VS ;
VALVI, FN .
ASTROPHYSICAL JOURNAL, 1987, 312 (01) :219-226
[8]   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
[9]   STRUCTURE + STABILITY OF ROTATING GAS MASSES [J].
JAMES, RA .
ASTROPHYSICAL JOURNAL, 1964, 140 (02) :552-&
[10]   THE VOLUME AND SURFACE-AREA OF A UNIFORMLY ROTATING POLYTROPE [J].
LINNELL, AP .
ASTROPHYSICS AND SPACE SCIENCE, 1981, 80 (02) :501-511