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

被引：16

作者：

GEROYANNIS, VS ^{[1
]}

VALVI, FN ^{[1
]}

机构：

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

来源：

关键词：

D O I：

10.1086/163735

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：695 / 705

页数：11

共 35 条

[1]

Aikawa T., 1968, Science Reports of the Tohoku University, First Series, V51, P61

ANAND, SPS .

[3]

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

[4]

Booth A. D., 1966, NUMERICAL METHODS, V3rd

CAIMMI, R .

[6]

CAIMMI R, 1980, ASTROPHYS SPACE SCI, V71, P415

[7]

CHANDRASEKHAR S, 1962, AP J, V137, P1082

[8]

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

[9]

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

CLEMENT, MJ .