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http://hdl.handle.net/2289/1574
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DC Field | Value | Language |
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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) |
Files in This Item:
File | Description | Size | Format | |
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1997_MNRAS_Vol.288_p565.pdf | Open Access | 893.22 kB | Adobe PDF | View/Open |
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