Pulsar Wind Nebulae and Their Supernovae

dc.creatorChevalier, Roger A.
dc.date2003-10-24
dc.date.accessioned2026-07-07T02:10:49Z
dc.date.available2026-07-07T02:10:49Z
dc.descriptionYoung supernova remnants that contain pulsar wind nebulae provide diagnostics for both the inner part of the supernova and the interaction with the surrounding medium, providing an opportunity to relate these objects to supernova types. Among observed young nebulae, there is evidence for a range of supernova types, including Type IIP (Crab Nebula and SN 1054) and Type IIb/IIn/IIL (G292.0+1.8).
dc.description4 pages, to appear in "Young Neutron Stars and Their Environments" (IAU Symposium 218, ASP Conference Proceedings), eds. F. Camilo and B. M. Gaensler
dc.identifierhttps://arxiv.org/abs/astro-ph/0310730
dc.identifierhttp://arxiv.org/abs/astro-ph/0310730
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6866
dc.subjectAstrophysics
dc.titlePulsar Wind Nebulae and Their Supernovae
dc.typetext

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