A model for the millisecond pulsar PSR 1937 + 214

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3978

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DC Field	Value	Language
dc.contributor.author	Kochhar, R. K	-
dc.contributor.author	Sivaram, C	-
dc.date.accessioned	2008-10-25T13:06:18Z	-
dc.date.available	2008-10-25T13:06:18Z	-
dc.date.issued	1984-01	-
dc.identifier.citation	Astrophysics and Space Science, Vol. 98, No. 1, pp. 201- 202	en
dc.identifier.issn	0004-640X	-
dc.identifier.uri	http://hdl.handle.net/2248/3978	-
dc.description.abstract	The authors suggest a model for the millisecond pulsar PSR 1937+214, according to which the immediate progenitor of the pulsar was a binary consisting of two neutron stars of unequal mass. The heavier neutron star was spun up by the transfer of angular momentum from the orbit, and the lighter neutron star was tidally disrupted, leaving behind a millisecond pulsar.	en
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.uri	http://www.springerlink.com/content/p586k232533274j5/	en
dc.subject	Astrophysics	en
dc.subject	Binary Stars	en
dc.subject	Pulsars	en
dc.subject	Stellar Models	en
dc.subject	Angular Momentum	en
dc.subject	Momentum Transfer	en
dc.subject	Neutron Stars	en
dc.subject	Stellar Mass Accretion	en
dc.title	A model for the millisecond pulsar PSR 1937 + 214	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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