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http://hdl.handle.net/2289/1599
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DC Field | Value | Language |
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dc.contributor.author | Srinivasan, G. | - |
dc.contributor.author | van den Heuvel, E.P.J. | - |
dc.date.accessioned | 2006-12-19T05:58:29Z | - |
dc.date.available | 2006-12-19T05:58:29Z | - |
dc.date.issued | 1982-04 | - |
dc.identifier.citation | Astronomy and Astrophysics, 1982, Vol.108, p143-147. | en |
dc.identifier.issn | 0004-6361 | - |
dc.identifier.uri | http://hdl.handle.net/2289/1599 | - |
dc.description.abstract | It is argued that the combination of 0.059 s pulse period and weak surface dipole magnetic field strength of PSR 1913 + 16 is excluded for a newly born pulsar. This yields support to the suggestion that PSR 1913 + 16 obtained its short pulse period during a spiral-in history, in which it underwent heavy accretion of matter with angular momentum from its companion. The shortest possible pulse period compatible with its magnetic field in such a case is approximately 0.04 s. As this spiral-in will have completely circularized the orbit, its presently large orbital eccentricity indicates that a second supernova explosion must have taken place in the system and, consequently, that its companion is also a neutron star (or a black hole). It is argued that the progenitor system was a binary with component masses of at least 8 solar masses. The various possible types of radio pulsars resulting from the evolution of close binaries are discussed. | en |
dc.format.extent | 812130 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Springer-Verlag | en |
dc.relation.uri | http://adsabs.harvard.edu/cgi-bin/bib_query?1982A&A...108..143S | en |
dc.rights | (1982) by the European Southern Observatory. Scanned images provided by the NASA ADS. | en |
dc.subject | Binary stars | en |
dc.subject | Neutron stars | en |
dc.subject | Pulsars | en |
dc.subject | Stellar evolution | en |
dc.subject | X-ray sources | en |
dc.subject | Angular momentum | en |
dc.subject | Roche limit | en |
dc.subject | Stellar magnetic fields | en |
dc.subject | Stellar mass accretion | en |
dc.title | Some constraints on the evolutionary history of the binary pulsar PSR 1913+16 | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
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1982 A&A V108 p143.pdf | 5p. | 793.1 kB | Adobe PDF | View/Open |
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