Kinematics of low-mass X-ray binaries and millisecond pulsars

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1574

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DC Field	Value	Language
dc.contributor.author	Ramachandran, R.	-
dc.contributor.author	Bhattacharya, D.	-
dc.date.accessioned	2006-12-13T11:23:10Z	-
dc.date.available	2006-12-13T11:23:10Z	-
dc.date.issued	1997-07	-
dc.identifier.citation	Monthly Notices of the Royal Astronomical Society, 1997, Vol.288, p565-571	en
dc.identifier.issn	0035-8711	-
dc.identifier.uri	http://hdl.handle.net/2289/1574	-
dc.description	Open Access	en
dc.description.abstract	The kinematic properties of low-mass X-ray binaries and millisecond pulsars have been studied with the help of a Monte Carlo simulation. It is found that the kinematic properties of these two populations are consistent with each other, which supports the idea that LMXBs are the progenitors of millisecond pulsars. The speed distribution of millisecond pulsars is seen to be quite different from that of ordinary pulsars.	en
dc.format.extent	8338 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Blackwell Publishing for the Royal Astronomical Society	en
dc.relation.uri	http://adsabs.harvard.edu/cgi-bin/bib_query?1997MNRAS.288..565R	en
dc.relation.uri	http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997MNRAS.288..565R&link_type=ARTICLE&db_key=AST	en
dc.rights	(1997) Royal Astronomical Society	en
dc.subject	Binaries	en
dc.subject	Stars:kinematics	en
dc.subject	Pulsars	en
dc.title	Kinematics of low-mass X-ray binaries and millisecond pulsars	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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