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