POST-NEWTONIAN EFFECTS ON THE MODES OF ROTATING STARS

被引：19

作者：

CUTLER, C ^{[1
]}

机构：

[1] UNIV PITTSBURGH,DEPT PHYS & ASTRON,PITTSBURGH,PA 15260

来源：

ASTROPHYSICAL JOURNAL | 1991年 / 374卷 / 01期

关键词：

RELATIVITY; STARS; PULSATION; ROTATION;

D O I：

10.1086/170113

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A formidable unsolved problem in general relativity is how to calculate the nonaxisymmetric pulsational modes of rotating stars. Even in Newtonian gravity, the mode equations for rotating stars have only recently been solved numerically by Ipser and Lindblom. In this paper we show how their Newtonian calculations may be easily extended to first post-Newtonian order.

引用

页码：248 / 254

页数：7

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