| 1. | Are some known neutron stars actually strange stars
一些已知的中子星会否就是奇异星？ |
| 2. | Are there strange stars
奇异星到底是否存在？ |
| 3. | This wrong discovery , however , promoted the progressive development in the field of strange star
虽然这个发现在一年后证实是错误的，但它却触发了对奇异星的研究。 |
| 4. | Due to the existence of high viscosity in strange matter , strange stars can reach much shorter period than neutron stars
由于奇异星有很高的粘度，它的自转周期会比中子星短得多。 |
| 5. | If the pulsar with submillisecond period would exist , it should be a strange star rather than a neutron star
如果一颗周期少于一毫秒的脉冲星真的存在的话，它便很可能会是一颗奇异星而不是中子星。 |
| 6. | However , it is now proposed that the conversion of neutron stars to strange stars is another possible origin of gamma - ray bursts
不过，近期有研究指出，伽玛射线爆发现象，也可能是由一颗中子星转变为奇异星时所产生的。 |
| 7. | 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
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。 |
| 8. | Although there are quite a number of evidences to support the strange stars , more detail studies in experiments and observations are necessary to make a very sound confirmation about their existence stars
虽然现时已有相当的理据支持奇异星的概念，但要证实奇异星的存在，还需要有更深入的研究和观测。 |
| 9. | Because the neutrino energy loss rate in strange matter is much higher than that in neutron matter , the surface temperature of a young strange star is lower than that of an ordinary neutron star of the same age
奇异星与中子星的表面热辐射特性有显著的不同。由于奇异物质发射较多中微子，所以能量损失速度较快，因此一颗年青的奇异星，表面温度会比同年的中子星为低。 |
| 10. | In 1986 , alcock et al . studied the structures of the strange stars . they found that a typical strange star basically consists of two components , a solid crust and a core filled with quarks which are likely superconducting liquid
1986年，艾确和他的同僚对奇异星的结构进行研究，发现一颗典型的奇异星，主要是由一个固体外壳和一个可能呈超导液体状态的夸克核心所构成。 |
