Origin of the proper motion and spin of pulsars

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DC Field	Value	Language
dc.contributor.author	Cowsik, R	-
dc.date.accessioned	2008-08-22T10:41:33Z	-
dc.date.available	2008-08-22T10:41:33Z	-
dc.date.issued	1998-12	-
dc.identifier.citation	Astronomy and Astrophysics, Vol. 340, No. 2, pp. L65 - L67	en
dc.identifier.issn	0004 - 6361	-
dc.identifier.uri	http://hdl.handle.net/2248/3256	-
dc.description.abstract	It is suggested that the proper motion and the spin of pulsars at birth are causally connected. Accordingly, the observed mean values of these parameters can be attributed to the recoil momentum and torque impulse imparted to the neutron star by anisotropic and asymmetric emission of neutrinos during the collapse of the core in a supernova.	en
dc.format.extent	77562 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	The European Southern Observatory	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1998A%26A...340L..65C	en
dc.subject	Pulsar	en
dc.subject	Spin	en
dc.subject	Proper Motion	en
dc.subject	Supernovae	en
dc.title	Origin of the proper motion and spin of pulsars	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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