现在，两个小组宣称他们掌握了这种中子星内奇异超流体的直接证据，并且其他研究者似乎相信这一发现。
Now, two teams say they have direct evidence of such bizarre "superfluidity" in a neutron star, and other researchers seem convinced.
奇异子会很慢的吞噬掉中子星（以上百万年甚至上亿年的缓慢速度），因为它发现中子真的很“美味”。
The Q-ball will slowly eat its heart out (very slowly, over millions or billions of years), because it finds neutrons so very tasty.
这个女孩长久地凝望着那颗星，她有了一种奇异的幻觉，好像启明星就是她的情人。
The girl looked long at the Star, and she had strange fancies, and imagined that he was her lover.
随着吉文人高度智慧化，他们完成了形式复杂的数学体系，以预测亚格杜尔星轨道上奇异的卫星系运动。
As the Givin developed intellectually, they perfected complex forms of mathematics to help predict the bizarre moon system orbiting Yag'Dhul.
本文用有效质量口袋模型描述夸克物质研究了流夸克质量的选取对奇异星性质的影响。
In this paper the influence of choice of the current quark mass on the properties of strange stars is studied by using the effective mass bag model to describe quark matter.
天文学家对它的能量持续时间间隔时间和光谱进行了研究，发现它可能是一颗正在吸取伴星物质的奇异星。
Study of the burst energy, duration, interval and spectrum suggested that this source could be a strange star accreting matter from its low - mass companion.
在我们介绍了磁场中夸克物质状态及奇异星的基本结构后，本文主要研究磁场在两个方面对奇异星的效应。
We introduced the state of strange quark matter and the structure of strange star in magnetic field, our paper was focus in the effect of magnetic on strange star in two sides.
因其色禁闭及小体积特点，低质量裸奇异星可以非常快地自转且几乎不受引力辐射不稳定性的约束。
Besides small thermal radii, low-mass quark stars could spin very fast, with a negligible effect of r-mode instability.
因其色禁闭及小体积特点，低质量裸奇异星可以非常快地自转且几乎不受引力辐射不稳定性的约束。
Besides small thermal radii, low-mass quark stars could spin very fast, with a negligible effect of r-mode instability.
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