Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Artemova, I. V."'
We consider the effects of advection and radial gradients of pressure and radial drift velocity on the structure of optically thick accretion disks. We concentrate our efforts on highly viscous disks, $\alpha=1.0$, with large accretion rates. Contrar
Externí odkaz:
http://arxiv.org/abs/astro-ph/9701140
We present solutions to the accretion disk structure equations in which advective cooling is accounted for in a self-consistent way. It is shown that for high rates of accretion, above a critical value, when without advection there are no solutions e
Externí odkaz:
http://arxiv.org/abs/astro-ph/9601008
We present here the solution for accretion disk structure, which describes continuously the transition between optically thick and optically thin disk regions. We show that the disk structure equations without advection, used here, give two branches
Externí odkaz:
http://arxiv.org/abs/astro-ph/9505051