| 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. | Though some ideas of quark stars were proposed as early as in 1969 , no great progress had been made until the 1980s
虽然天文学家早在1969年便提出奇异星的概念，但直至80年代，这个理论才有更进一步的发展。 |
| 7. | 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。 |
| 8. | 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。 |
| 9. | 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。 |
| 10. | 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。 |
