• 主题
高级搜索  >
历史搜索 清空历史
首页> 外文期刊>International Journal of Modern Physics, A. Particles and Fields, Gravitation, Cosmology >On the theory of gamma ray bursts and hypernovae: The black hole soft X-ray transient sources [Review]
【24h】

On the theory of gamma ray bursts and hypernovae: The black hole soft X-ray transient sources [Review]

机译：关于伽马射线爆发和超新星的理论：黑洞软X射线瞬变源[综述]

获取原文
获取原文并翻译 | 示例
           
页面导航
  • 摘要
  • 著录项
  • 相似文献
  • 相关主题

摘要

We show that a common evolutionary history can produce the black hole binaries in the Galaxy in which the black holes have masses of similar to 5 - 10M(circle dot). In the black hole binaries with low-mass, less than or similar to 2.5M(circle dot), ZAMS (zero age main-sequence) companions, the latter remain in main sequence during the active stage of soft X-ray transients (SXT's), most of them being of K or M classification. In two intermediate cases, IL Lupi and Nova Scorpii with ZAMS similar to 2.5M(circle dot) companions the orbits are greatly widened because of large mass loss in the explosion forming the black hole, and whereas these companions are in late main sequence evolution, they are close to evolving. Binaries with companion ZAMS masses greater than or similar to 3M(circle dot) are initially "silent" until the companion begins evolving across the Herzsprung gap. We provide evidence that the narrower, shorter period binaries, with companions now in main sequence, are fossil remnants of gamma ray bursters (GRB's). We also show that the GRB is generally accompanied by a hypernova explosion (a very energetic supernova explosion). We further show that the binaries with evolved companions are good models for some of the ultraluminous X-ray-sources (ULX's) recently seen by Chandra in other galaxies. The great regularity in our evolutionary history, especially the fact that most of the companions of ZAMS mass less than or similar to 2.5M(circle dot) remain in main sequences as K or M stars can be explained by the mass loss in common envelope evolution to be Case C; i.e. to occur only after core He burning has finished. Since our argument, for Case C mass transfer is not generally understood in the community, we add an appendix, showing that with certain assumptions which we outline we can reproduce the regularities in the evolution of black hole binaries by Case C mass transfer. [References: 123]
机译：我们证明了一个共同的进化史可以在银河系中产生黑洞双星，其中黑洞的质量类似于5-10M（圆点）。在质量小于或等于2.5M（圆点）的ZAMS（零年龄主序列）伴星的低质量黑洞双星中，后者在软X射线瞬变（SXT's）的活动阶段保持主序列。 ），其中大多数属于K或M分类。在两种中间情况下，IL Lupi和Nova Scorpii的ZAMS类似于2.5M（圆点）伴星，由于形成黑洞的爆炸中的大量质量损失，使轨道大大加宽，而这些伴星处于主序列晚期演化，他们即将发展。伴随ZAMS质量大于或等于3M（圆圈点）的二进制文件最初是“静默的”，直到伴侣开始跨越Herzsprung间隙演化。我们提供的证据表明，更窄，更短的二进制文件，以及现在处于主要序列中的同伴，是伽马射线爆发器（GRB's）的化石残余。我们还显示，GRB通常伴随着超新星爆炸（非常活跃的超新星爆炸）。我们进一步证明，带有演化伴星的二进制文件是钱德拉在其他星系中最近发现的一些超发光X射线源（ULX）的良好模型。我们进化史上的规律性很强，尤其是大多数ZAMS质量小于或等于2.5M（圆点）的ZAMS伴星仍保留在主要序列中，因为K或M星可以用共同包络演化中的质量损失来解释。属于情况C;即仅在核心He燃烧结束后才发生。由于我们的论点是，对于社区中通常不了解Case C传质的问题，我们添加了一个附录，该附录表明，通过概述某些假设，我们可以再现Case C传质在黑洞二元演化过程中的规律性。 [参考：123]

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱：kefu@zhangqiaokeyan.com

京公网安备：11010802029741号 ICP备案号：京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有

  • 客服微信

  • 服务号