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Are Most of X-Ray Binaries Recurrent Transients?
Published online by Cambridge University Press: 14 August 2015
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The aim of this paper is to argue that some day in the not-too-distant future one of the well-known X-ray pulsars, say, Cen X-3 (although better examples would be probably GX 301-2 or GX 1+4), will disappear from the X-ray sky. It will reappear again after some, say, tens of years and its pulse period will be then longer than it is now.
- Type
- VI. X-Ray Binaries
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- Copyright © Reidel 1980
References
Davies, R.E., Fabian, A.C. and Pringle, J.E.: 1979, Monthly Notices Roy. Astron. Soc.
186, p. 779.Google Scholar
Giangrande, A., Giovanelli, F., Bartolini, C., Guarnieri, A. and Piccioni, A.: 1978, preprint.Google Scholar
Lamb, F.K.: 1977, in
Eight Texas Symposium on Relativistic Astrophysics
, Annals New York Academy Sciences
302, p. 482.Google Scholar
Li, F., Rappaport, S., Clark, G.W. and Jernigan, J.G.: 1979, Astrophys. J.
228, p. 893.Google Scholar
Sanford, P.W.: 1977, in
Eight Texas Symposium on Relativistic Astrophysics
, Annals New York Academy Sciences
302, p. 386.CrossRefGoogle Scholar
Schreier, E.J.: 1977, in
Eight Texas Symposium on Relativistic Astrophysics
, Annals New York Academy Sciences
302, p. 445.Google Scholar
van den Heuvel, E.P.J.: 1977, in
Eight Texas Symposium on Relativistic Astrophysics
, Annals New York Academy Sciences
302, p. 14.CrossRefGoogle Scholar
Ziółkowski, J.: 1977, in
Eight Texas Symposium on Relativistic Astrophysics
, Annals New York Academy Sciences
302, p. 47.Google Scholar
Ziółkowski, J.: 1978, in
Nonstationary Evolution of Close Binaries
, ed. Zytkow, A.N. (Warsaw: Polish Scientific Publishers), pp. 29–54.Google Scholar
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