结果表明夸克星的质量分布在事件视界以内，即夸克星是黑洞，但构成这种黑洞的物质并没有坍缩到大小为零的一点。
That is , a quark star is a black hole, while the black hole formation has not collapsed to one point yet.
因质量的大小而形成脉冲星、中子星、夸克星，质量大到一定值的生成黑洞。
Pulsars, neutron stars and quark stars are then created based on their mass.
文章估算了夸克星的质量极限和半径。
This article estimates the mass limit, degeneration and radius of quark stars.
简要地回顾了脉冲星、中子星和夸克星的研究历史；
Studies of pulsars, neutron stars, and quark stars are reviewed.
关于观测到脉冲星的本质目前存在两种看法：中子星和夸克星。
Neutron stars and quark stars are currently two kinds of speculated subjects when one is modeling observed pulsars.
给出了一些夸克星候选体以及未来可能的观测检验。
Quark star candidates are suggested, which could be tested by future observations.
给出了一些夸克星候选体以及未来可能的观测检验。
Quark star candidates are suggested, which could be tested by future observations.
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