光学观测孤立中子星的意义
天体物理学
2007-05-23 v1
摘要
对5颗已确认的光学脉冲星的观测表明，峰值发射强度随外场强度而变化。我们证明这进一步确认了Pacini和Salvati (1987)等简单现象模型仍具有有效性。此外，我们指出，蟾蜍脉冲星显示出非脉冲发射，这进一步复杂化了对孤立中子星热发射的研究。
引用
@article{arxiv.astro-ph/9912057,
title = {Implications of the Optical Observations of Isolated Neutron Stars},
author = {Andy Shearer and Aaron Golden and Gregory Beskin},
journal= {arXiv preprint arXiv:astro-ph/9912057},
year = {2007}
}
备注
4 pages, 3 figures, to appear in the Proceedings of IAU Colloquium 177 : "Pulsar Astronomy - 2000 & Beyond", Ed. Kramer, Wex & Wielebinski, ASP conf.Series. Uses newpasp.sty