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GRAVITATIONAL-RADIATION AND SPIRALING TIME OF CLOSE BINARY-SYSTEMS (V)

被引：0
|
作者：
PADALIA, TD
机构：
[1] Uttar Pradesh State Observatory, Manora Peak, Naini Tal
来源：
ASTROPHYSICS AND SPACE SCIENCE | 1993年 / 202卷 / 01期
关键词：
D O I：
10.1007/BF00626916
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Forty-six binary systems with their primary component masses between 2 M. and 3 M. have been considered for gravitational radiation study. Power output by gravitational radiation (P(B)) and spiral time tau0 for all individual systems have been evaluated. A relation has been given between P(B) and tau0. The rate of decrease of orbital period (P) has also been given for 10 eccentric orbit systems.
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页码：63 / 68
页数：6
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