Neutron Stars in Supernova Remnants

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dc.creatorPacini, Franco
dc.date1999-11-22
dc.date.accessioned2026-07-07T02:34:36Z
dc.date.available2026-07-07T02:34:36Z
dc.descriptionI briefly summarize some facts and ideas concerning the presence of neutron stars in Supernova remnants. While sources similar to the Crab Nebula require the presence of a central energetic object, shell-type remnants such as Cas A are compatible with the presence of neutron stars releasing a weak relativistic wind.
dc.description3 pages, to be published in proceedings of ``Highly Energetic Physical Processes and Mechanisms for Emission from Astrophysical Plasmas'', ASP Conf. Ser
dc.identifierhttps://arxiv.org/abs/astro-ph/9911418
dc.identifierhttp://arxiv.org/abs/astro-ph/9911418
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15305
dc.subjectAstrophysics
dc.titleNeutron Stars in Supernova Remnants
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