Relativistic Milne-Eddington Type Solutions with a Variable Eddington Factor for Relativistic Spherical Winds
Figure 4
Comoving luminosity for relativistic spherical flows in the LTE case with a uniform source function. The values of are from 0 to 0.9 in steps of 0.1 from top to bottom. The optical depth at the core radius is set to be 10, and the value of the source function is set to be unity. The solid curves represent the present analytical solutions, while the dashed ones mean the solutions of the homogeneous part.
