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http://hdl.handle.net/2289/2427
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DC Field | Value | Language |
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dc.contributor.author | Radhakrishnan, V. | - |
dc.contributor.author | Srinivasan, G. | - |
dc.date.accessioned | 2007-05-25T08:45:34Z | - |
dc.date.available | 2007-05-25T08:45:34Z | - |
dc.date.issued | 1983 | - |
dc.identifier.citation | IAU Symposium, 1983, Vol.101, p487-494 | en |
dc.identifier.uri | http://hdl.handle.net/2289/2427 | - |
dc.description | Open Access. Supernova remnants and their X-ray emission; Proceedings of the Symposium, Venice, Italy, August 30-September 2, 1982 (A84-43078 21-90). Dordrecht, D. Reidel Publishing Co., 1983 | en |
dc.description.abstract | Available data on associations between pulsars and supernova remnants (SNR) are surveyed for possible conclusions that may be drawn. Pulsars have been detected in the Crab and Vela SNR. The pulsar in Vela is at the periphery of the nebula at the edge of the shell, whereas the shell energy may be derived from other neutron stars in Vela. Calculations of the pulsar birthrate are consistent with the current discovery rate and birthrate of SNRs. It is possible that all SN produce pulsars, some which never reach a detectable, active stage. Finally, the Crab Nebula is regarded as an atypical situation. | en |
dc.format.extent | 865798 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Reidel | en |
dc.relation.uri | http://adsabs.harvard.edu/cgi-bin/bib_query?1983IAUS..101..487R | en |
dc.rights | 1983 Reidel | en |
dc.subject | Pulsars | en |
dc.subject | Supernova Remnants | en |
dc.subject | Crab nebula | en |
dc.subject | Neutron stars | en |
dc.title | On the association between pulsars and supernova remnants | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
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1983 IAU Symp V101 p487.pdf Restricted Access | Open Access | 845.51 kB | Adobe PDF | View/Open Request a copy |
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