Whither strange pulsars?

dc.contributor.author	Konar, S
dc.date.accessioned	2008-03-03T10:02:27Z
dc.date.available	2008-03-03T10:02:27Z
dc.date.issued	2000
dc.identifier.citation	BASI, Vol. 28, No. 2, pp. 299 - 301	en
dc.identifier.uri	http://hdl.handle.net/2248/2108
dc.description.abstract	It has been argued that some of the pulsars could be strange stars because these too are capable of supporting fast rotations observed in pulsars. We examine this claim from the point of view of the evolution of magnetic field in pulsars and find that there is no compelling reason for the existence of strange pulsars.	en
dc.format.extent	188872 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2000BASI...28..299K	en
dc.subject	Magnetic fields	en
dc.subject	Stars-neutron	en
dc.subject	Stars-strange	en
dc.subject	Pulsars-general	en
dc.title	Whither strange pulsars?	en
dc.type	Article	en