Pulse emission mechanisms

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High-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.
To appear in "Young Neutron Stars and Their Environments" (IAU Symposium 218, ASP Conference Proceedings), eds F. Camilo and B. M. Gaensler

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/6390

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/0308471
 http://arxiv.org/abs/astro-ph/0308471

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arXiv