Stars can live for billions of years. A star is born when an enormous cloud of hydrogen gas collapses until it is hot enough to burn nuclear fuel (producing tremendous amounts heat and radiation). As the nuclear fuel runs out (in about 5 billion years), the star expands and the core c...
An All-Union Seminar on the Physics of Neutron Stars was held at the Ioffe Physial-Technical Institute from March 15 to 18, 1988. Papers presented at this seminar are briefly reviewed, with attention given to the following topics: neutron-star (NS) formation and structure; NS evolution in ...
Gravitational-wave measurements of the tidal deformability of neutron stars could reveal important information regarding their internal structure, the equation of state of high-dense nuclear matter and gravity in strong field regime. In this work, we extend the relativistic theory of the tidal deformabi...
All in the timing: Taking a tape measure to neutron starsdoi:10.2307/4010871RonCowenWileyScience News
of years ago. As a result, the galaxy is bristling with star formation and long, delicate-looking streamers of dust threading through the arms. It also has a supermassive black hole at its heart, and there are other smaller black holes and neutron stars scattered throughout its spiral arms....
X-RAY-EMITTING STARS IDENTIFIED FROM THE ROSAT ALL-SKY SURVEY AND THE SLOAN DIGITAL SKY SURVEYIncludes observations obtained with the Apache Point Observatory 3.5 m telescope, which is owned and operated by the Astrophysical Research Consortium. ...
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【24h】 Candidate isolated neutron stars and other stellar X -ray sources from the ROSAT All-Sky and Sloan Digital Sky Surveys. 机译:候选孤立的中子星和其他ROSAT全天和斯隆数字天空测量的X射线源。 获取原文 获取原文并翻译|示例 著录项 作者
根据第三段关键句“When the temperature inside the clouds climbs to about 15 million degrees Celsius, nuclear fusion (核聚变) starts and they enter the next stage of life, known as main sequence. Stars spend 90 percent of their lives in their main sequence phase. Most of the stars, ...
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