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

Title: Kinematics of low-mass X-ray binaries and millisecond pulsars
Authors: Ramachandran, R.
Bhattacharya, D.
Keywords: BINARIES: CLOSE,
STARS: KINEMATICS,
PULSARS: GENERAL
Issue Date: Jul-1997
Publisher: Blackwell Publishing for the Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, 1997, Vol.288, p565-571
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.
Description: Sorry, the full text of this article is not available here. Please click on the alternative location to access it.
URI: http://hdl.handle.net/2289/1574
ISSN: 0035-8711
Alternative Location: http://adsabs.harvard.edu/cgi-bin/bib_query?1997MNRAS.288..565R
http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997MNRAS.288..565R&link_type=ARTICLE&db_key=AST
Copyright: (1997) Royal Astronomical Society
Appears in Collections:Research Papers (A&A)

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