Journal
ASTRONOMY & ASTROPHYSICS
Volume 449, Issue 2, Pages 443-447Publisher
EDP SCIENCES S A
DOI: 10.1051/0004-6361:20053997
Keywords
accretion, accretion disks; black hole physics; X-rays : binaries; cooling flows
Categories
Ask authors/readers for more resources
Heat conduction plays an important role in the balance between heating and cooling in many astrophysical objects, e. g. cooling flows in clusters of galaxies. Here we investigate the effect of heat conduction on the interaction between a cool disk and a hot corona around black holes. Using the one-radial-zone approximation, we study the vertical structure of the disk corona and derive evaporation and coronal mass flow rates for various reduced thermal conductivities. We find lower evaporation rates and a shift in the evaporation maxima to smaller radii. This implies that the spectral state transition occurs at a lower mass flow rate and a disk truncation closer to the black hole. Reductions of thermal conductivity are thought to be magnetically caused and might vary from object to object by a different configuration of the magnetic fields.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available