Gravitational radiation and spiralling time of close binary systems (V) |
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| Authors: | T D Padalia |
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| Institution: | (1) Uttar Pradesh State Observatory, Manora Peak, Naini Tal, India |
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| Abstract: | Forty-six binary systems with their primary component masses between 2M
 and 3M
have been considered for gravitational radiation study. Power output by gravitational radiation (P
B
) and spiral time
0 for all individual systems have been evaluated. A relation has been given betweenP
B
and
0. The rate of decrease of orbital period (P) has also been given for 10 eccentric orbit systems. |
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| Keywords: | |
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