摘要

In this work we study the density change along the accretion and wind branches when a modified Chaplygin gas is taken to be the accreting fluid. We get a high wind density very near to the black hole whereas we get a low wind density far from the black hole. In the modified Chaplygin gas accretion case a local minimum in the accretion density is got which can be detected as the CENBOL.

  • 出版日期2011-11