On the Association between Supernova Remnants and Pulsars
作者： D. Bhattacharya , G. Srinivasan
DOI: 10.1007/978-94-009-3823-6_11
关键词: Neutron star 、 Near-Earth supernova 、 Astronomy 、 Supernova 、 Stellar evolution 、 Pulsar 、 Crab Nebula 、 Supernova remnant 、 Stellar rotation 、 Physics 、 Astrophysics
摘要: From the extremely poor association between pulsars and supernova remnants, paucity of centrally filled synchrotron nebulae, presumably produced by active pulsars, we conclude that majority neutron stars must be born spinning rather slowly, with initial rotation periods ≳ 100 milliseconds.
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