Self Gravitating Accretion Disks - is the Temperature Independent of the Radius

Details Self Gravitating Accretion Disks - is the Temperature Independent of the Radius Self Gravitating Accretion Disks - is the Temperature Independent of the Radius

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987atsir1523....1l&link_type=abstract

Astronomicheskii Tsirkulyar NO. 1523/DEC, P. 1, 1987

Computer Science

Sound

Scientific paper

The structure of selfgravitating disks around supermassive black holes is considered. The temperature of the central plane of the disk is shown to be independent of the distance from the central object if η ≈ αρVsH. In this case the expression for the sound velocity involves combination of two-dimensional parameters - an accretion rate and the gravitational constant. The massive stars can be formed due to gravitational instability. Explosions of supernovae may lead to the disk destruction and vanishing of the nuclear activity.

Affiliated with

Also associated with

No associations

Rating

Self Gravitating Accretion Disks - is the Temperature Independent of the Radius does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Self Gravitating Accretion Disks - is the Temperature Independent of the Radius, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Self Gravitating Accretion Disks - is the Temperature Independent of the Radius will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-901480