Binary period decrease by unstable orbit

Details Binary period decrease by unstable orbit Binary period decrease by unstable orbit

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984aipc..115..143s&link_type=abstract

AIP Conference Proceedings, Volume 115, pp. 143-145 (1984).

Physics

X-Ray Binaries, Pulsars

Scientific paper

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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