THE STROBOSCOPIC METHOD APPLIED TO THE STELLAR 3-BODY PROBLEM - THE KEPLERIAN OUTER ORBIT APPROXIMATION

被引：2

作者：

LING, JF ^{[1
]}

DOCOBO, JA ^{[1
]}

ABAD, AJ ^{[1
]}

机构：

[1] UNIV ZARAGOZA,MECAN ESPACIAL GRP,E-50009 ZARAGOZA,SPAIN

来源：

ASTRONOMICAL JOURNAL | 1995年 / 110卷 / 02期

关键词：

D O I：

10.1086/117570

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

This article discusses the stellar three-body problem using an approximation in which the outer orbit is assumed to be Keplerian. The equations of motion are integrated by the stroboscopic method, i.e., basically at successive periods of a rapidly changing variable (the eccentric anomaly of the inner orbit). The theory is applied to the triple-star system xi Ursae Majoris. (C) 1995 American Institute of Physics.

引用

页码：875 / 879

页数：5

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