Towards a consistent model for Neutron-Star Sources
Astrophysics
2007-05-23 v1
Abstract
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.
Cite
@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}
}
Comments
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