On the implication of the recently discovered 5 millisecond binary pulsar PSR 1855+09

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1084

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DC Field	Value	Language
dc.contributor.author	Bhattacharya, D.	-
dc.contributor.author	Srinivasan, G.	-
dc.date.accessioned	2006-01-04T10:52:16Z	-
dc.date.available	2006-01-04T10:52:16Z	-
dc.date.issued	1986-04-05	-
dc.identifier.citation	Current Science, 1986, Vol. 55, p327-330.	en
dc.identifier.issn	0011-3891	-
dc.identifier.uri	http://hdl.handle.net/2289/1084	-
dc.description.abstract	We argue that the extraordinary fact that all three known millisecond pulsars are very close to the galactic plane implies that there must be ~100 potentially observable millisecond pulsars within ~ 4 kpc from the Sun. Our other main conclusion is that the dipole magnetic fields of old neutron stars probably saturate around 5 x l0^8 gauss.	en
dc.format.extent	265748 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences, Bangalore, India.	en
dc.rights	Indian Academy of Sciences, Bangalore, India.	en
dc.title	On the implication of the recently discovered 5 millisecond binary pulsar PSR 1855+09	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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