【摘要】 通过反投影分析方法 ,对XMM Newton观测的Abell 1835的数据进行分析 ,研究星系团中心的X射线性质 :温度成分及分布 ,冷流 ,强引力透镜 (r≈ 15 3kpc)的质量 ,星系团的总质量 ,投影质量 ,并与弱引力透镜质量进行了比较 .更多还原

【Abstract】 Through a detailed deprojection analysis of Abell 1835 observed by XMM-Newton, the X-ray property in the cluster is presented, including temperature, abundance, cooling flow rate, projected mass and total mass. It can be found that the projected mass within the strong lensing arc (～153 kpc) is only about half of the lensing mass, while on the large scale, the total projected mass is consistent with the weak lensing mass.更多还原