论文标题
在SRG/Erosita处孤立的中子星的可观察性
Observability of isolated neutron stars at SRG/eROSITA
论文作者
论文摘要
在船上使用Erosita望远镜的四年来调查，SPEKTR-RG天文台将在敏感性和角度分辨率方面提供柔软（0.5-2 KEV）和标准（2-10 KEV）X射线范围的最佳覆盖范围。我们已经分析了用Erosita检测各种类型的孤立的中子星的可能性。在已经有已知的物体中，Erosita将能够检测到160多个脉冲星，21个磁铁，7个中央紧凑型物体，宏伟的七个七个来源以及在四年的调查任务中其他两个X射线隔离的中子星。
A four-year sky survey with the use of the eROSITA telescope on board the Spektr-RG observatory will provide the best coverage in the soft (0.5-2 keV) and standard (2-10 keV) X-ray ranges, both in terms of sensitivity and angular resolution. We have analysed the possibility of detecting various types of isolated neutron stars with eROSITA. Among already known objects, eROSITA will be able to detect more than 160 pulsars, 21 magnetars, 7 central compact objects, all seven sources of the Magnificent Seven, and two other X-ray isolated neutron stars during the four-year survey mission.
