【摘要】 本文用广义相对论讨论了球状星团中荷磁黑洞附近星的投影密度分布,得到（dN/dΩ）_qm<（dN/dΩ）_s,即在中心是荷磁黑洞的球状星团中每单位立体角的星数少于中心是Schwarzschild黑洞的星数。更多还原

【Abstract】 The density distribution of the star numbers near to the magnetic black—hole in the globular custer is calculated in general relativity.（dN/dΩ）_qm <（dN/dΩ）_s is obtained, i.e., the star numbers per unit cubic angle in the globular custer with a magnetic black—hole are less than those with a schwarzschild black—hole.更多还原