The Problem of the Flickering Activity of the Recurrent Nova T CrB

摘要

On the basis of our previous paper (Hric et al. 1998) we can proclaim that the existence of two emission-line regions can remarkably affect the flickering activity in the binary system. We could expect flickering activity dependence on the orbital phase. Deriving the energy of the flickering and comparing the derived value with the energy particularly needed for three possible area where the source of the flickering could be settled down, we found the most plausible area to be in the unstable accretion onto the white dwarf, i.e. the boundary layer.