From low-mass X-ray binaries to binary and millisecond pulsars

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2681

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DC Field	Value	Language
dc.contributor.author	Bhattacharya, D.	-
dc.date.accessioned	2007-06-11T08:44:07Z	-
dc.date.available	2007-06-11T08:44:07Z	-
dc.date.issued	1992	-
dc.identifier.citation	Proceedings of the NATO ASI on X-ray binaries and recycled pulsars. 1991, Santa Barbara. Eds. E. P. J. van. den. Heuvel & S. A. Rappaport, p257, Kluwer, 1992, p257-268	en
dc.identifier.uri	http://hdl.handle.net/2289/2681	-
dc.description	Restricted Access.	en
dc.description.abstract	We review the origin of millisecond pulsars and low-mass binary pulsars &om low- mass X-ray binaries. Observations of such pulsars suggest that the existing evolutionary picture of low-mass X-ray binaries need major modifications. In particular, careful account has to be taken of the effect of the irradiation of the secondary star by high-energy radiation during the accretion phase, and by the radiation and particle wind from the pulsar after accretion ceases. Another element that has to be incorporated into this picture is the influence of accretion onto the neutron star and its spin evolution on its magnetic field strength.	en
dc.format.extent	603946 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Kluwer	en
dc.rights	1992 Kluwer	en
dc.title	From low-mass X-ray binaries to binary and millisecond pulsars	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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