Pulse emission mechanisms

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dc.creatorMelrose, Don
dc.date2003-08-27
dc.date.accessioned2026-07-07T02:09:19Z
dc.date.available2026-07-07T02:09:19Z
dc.descriptionHigh-energy and radio emission mechanisms for pulsars are reviewed. The source region for high energy emission remains uncertain. Two preferred radio emission mechanism are identified. Some difficulties may be resolved by appealing to nonstationary pair creation distributed widely in height.
dc.descriptionTo 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/0308471
dc.identifierhttp://arxiv.org/abs/astro-ph/0308471
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6390
dc.subjectAstrophysics
dc.titlePulse emission mechanisms
dc.typetext

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