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Binary period decrease by unstable orbit

 

作者: N. Shibazaki,   K. Makishima,   H. Inoue,   T. Murakami,  

 

期刊: AIP Conference Proceedings  （AIP Available online 1984）
卷期: Volume 115, issue 1  

页码: 143-145

 

ISSN:0094-243X

 

年代: 1984

 

DOI:10.1063/1.34516

 

出版商: AIP

 

数据来源: AIP

 

摘要:

The orbital period change due to unstable binary orbit has been examined for 6 binary x‐ray pulsars. It is shown that the orbital period decrease in Cen X‐3 is interpreted by this mechanism. SMCX‐1 is the next candidate for the unstable orbit, but more observations are necessary to reach the conclusion.

 

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