x-ray binary造句

• X - ray binaries
  X射线双星
• An x - ray binary system has been formed , and the neutron star has made the crucial second step toward becoming a millisecond pulsar
  射线双星就这样形成了，于是这颗中子星就向成为毫秒脉冲星迈出了关键的第二步。
• Astronomers are almost sure that the dark companions of many x - ray binaries are black holes and not neutron stars . v404 cygni is one of the most well - known examples
  天文学家已经几乎可以肯定很多x射线双星所包含的黑暗天体是黑洞而非中子星，其中最著名的例子包括天鹅座v404等。
• They suggest that these similarities between a known millisecond pulsar and a known x - ray binary provide the long - sought link between these types of objects
  他们认为，一个已知的毫秒脉冲星与一个已知的x射线双星之间的这种相似性，为我们提示了这两类天体间长期未知的内在联系。
• It links a millisecond pulsar with many of the properties of an x - ray binary , to j1808 , an x - ray binary that behaves in many ways like a millisecond pulsar , thus providing a strong chain of evidence to support the theory
  然而直到目前，决定性的证据还未获得，因为介于第一和第二步之间的过渡天体还几乎不为人所知。
• Most astronomers accept the binary spin - up scenario for creating millisecond pulsars because they have observed neutron stars speeding up in x - ray binary systems , and almost all radio millisecond pulsars are observed to be in binary systems
  多数天文家接受这个假想的模式，因为他们已经在x射线双星系统中观测到了中子星的加速现象，而且几乎所有的毫秒脉冲星都被发现时处于双星系统中。
• Recent study of the kilohertz quasi - periodic oscillations ( qpos ) in low mass x - ray binaries ( lmxbs ) indicates that the radiation force , other than the magnetosphere and disk interaction and the general relativity ( gr ) effect setting the inner disk edge , serves as the disk truncation mechanism on shorter time scales . some results and discussions are presented in this paper
  最近对低质量x射线双星中的千赫兹准周期振动的研究表明,是辐射压力,而不是盘和磁球的相互作用以及处于盘内边界的广义相对论效应在短时标的盘切断机制上起作用.本文给出了一些研究结果及讨论
• Such a process can take place in the low mass x - ray binary systems where the mass transfer from the companion to the neutron star can be larger than 0 . 5 solar masses . if the neutron star in the low mass x - ray binary accretes the matter , the central densities can reach to a state that strange - matter seeds are formed in the interiors of the star
  在这个系统内，中子星可能会吞噬超过0 . 5个太阳质量的伴星物质，当中子星吸收了这些物质后，中心的密度会增加至足以产生奇异物质种子，这些种子会开始吞噬四周的中子物质，释放出大量中微子和反中微子，令星体冷却。