A dynamical model of radiating stars and their thermal behavior

In this paper, we have studied a new class dynamical model of spherically symmetric radiating collapsing stars. The solution of field equations has been discussed by using the boundary condition and obtained all the physical parameters in terms of mass M and surface radius R${}_0$ which will be significant in astrophysical applications. We have also studied the thermal behavior of the stars and discussed the horizon formation and its temperature. We have shown that horizon temperature increases with time under certain conditions.