Towards a consistent model for Neutron-Star Sources
天体物理学
2007-05-23 v1
摘要
We are still far from understanding how pulsars pulse, how neutron stars are born, what neutron stars can emit, and in which way they do this. In this short communication, I list 18 alternatives -- several of them old, a few of them new -- which are handled differently by different authors but all of which are crucial for a model of neutron stars to be viable.
引用
@article{arxiv.astro-ph/0208570,
title = {Towards a consistent model for Neutron-Star Sources},
author = {W. Kundt},
journal= {arXiv preprint arXiv:astro-ph/0208570},
year = {2007}
}
备注
4 pages. To appear in the Proceedings of the 270. WE-Heraeus Seminar on Neutron Stars, Pulsars and Supernova Remnants, Jan. 21-25, 2002, Physikzentrum Bad Honnef, eds W. Becker, H. Lesch & J. Truemper. Proceedings are available as MPE-Report 278