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A Model of the Vela Supernova Remnant |
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| Authors: | Vasilii Gvaramadze |
| Institution: | (1) Abastumani Astrophysical Observatory, Georgian Academy of Sciences, A.Kazbegi ave. 2-a, Tbilisi, 380060, Georgia;(2) Sternberg State Astronomical Institute, Universitetskij Prospect 13, Moscow, 119899, Russia;(3) Abdus Salam International Centre for Theoretical Physics, Strada Costiera 11, P.O. Box 586, 34100 Trieste, Italy |
| Abstract: | A model of the Vela supernova remnant (SNR) based on a cavity explosion of a supernova (SN) star is proposed. It is suggested that the general structure of the remnant is determined by the interaction of the SN blast wave with a massive shell created by the SN progenitor (15-20 M⊙) star. A possible origin of the nebula of hard X-ray emission detected around the Velapulsar is discussed. This revised version was published online in July 2006 with corrections to the Cover Date. |
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