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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2427

Title: On the association between pulsars and supernova remnants
Authors: Radhakrishnan, V.
Srinivasan, G.
Keywords: PULSARS
SUPERNOVA REMNANTS
CRAB NEBULA
NEUTRON STARS
Issue Date: 1983
Publisher: Reidel
Citation: IAU Symposium, 1983, Vol.101, p487-494
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.
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
URI: http://hdl.handle.net/2289/2427
Alternative Location: http://adsabs.harvard.edu/cgi-bin/bib_query?1983IAUS..101..487R
Copyright: 1983 Reidel
Appears in Collections:Research Papers (A&A)

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