Pulse emission mechanisms
Astrophysics
2007-05-23 v1
Abstract
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.
Cite
@article{arxiv.astro-ph/0308471,
title = {Pulse emission mechanisms},
author = {Don Melrose},
journal= {arXiv preprint arXiv:astro-ph/0308471},
year = {2007}
}
Comments
To appear in "Young Neutron Stars and Their Environments" (IAU Symposium 218, ASP Conference Proceedings), eds F. Camilo and B. M. Gaensler