`Bare' Strange Stars Might Not Be Bare
`Bare' Strange Stars Might Not Be Bare
复制标题
DOI：
10.1088/0256-307x/15/12/026
复制
发表时间：
1998-11
影响因子：
3.5
通讯作者：
R. Xu;G. J. Q. D. O. Geophysics;Peking University;Beijing;P. China;Ccast;P. R.China;CAS-PKU Joint Beijing Astrophysics Center
中科院分区：
文献类型：
--
作者：
R. Xu;G. J. Q. D. O. Geophysics;Peking University;Beijing;P. China;Ccast;P. R.China;CAS-PKU Joint Beijing Astrophysics Center
有人提出，“裸露”的奇怪物质恒星可能不是裸露的，而观测到的脉冲星可能实际上是“裸露”的奇怪恒星。当被强烈磁化的奇异物质恒星旋转时，产生的单极电场大到足以形成磁球。这种情况与许多作者对旋转中子星的讨论非常相似。此外，在双星中有吸积壳的奇怪恒星可以作为x射线脉冲星或x射线爆发星。如果脉冲星是“光秃秃”的奇怪恒星，那就有一些优势。
It is proposed that the `bare' strange matter stars might not be bare, and the observed pulsars might be in fact the `bare' strange stars. As intensely magnetized strange matter stars rotate, the induced unipolar electric fields would be large enough to construct magnetospheres. This situation is very similar to that discussed by many authors for rotating neutron stars. Also, the strange stars with accretion crusts in binaries could act as x-ray pulsars or x-ray bursters. There are some advantages if pulsars are `bare' strange stars.