Towards a consistent model for Neutron-Star Sources
| dc.creator | Kundt, W. | |
| dc.date | 2002-08-30 | |
| dc.date.accessioned | 2026-07-07T02:04:53Z | |
| dc.date.available | 2026-07-07T02:04:53Z | |
| dc.description | 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. | |
| dc.description | 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 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0208570 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0208570 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/4933 | |
| dc.subject | Astrophysics | |
| dc.title | Towards a consistent model for Neutron-Star Sources | |
| dc.type | text |