Collisionless Halos Around Black Holes

Details Collisionless Halos Around Black Holes Collisionless Halos Around Black Holes

1999-08-04

arxiv.org/abs/astro-ph/9908027v1

Astronomy and Astrophysics

Astrophysics

7 pages, Proceedings IAU Symposium 195

Scientific paper

When a black hole accretes slowly, the radiative cooling of the infalling gas
is weak and the accretion disk does not form. A hot collisionless
quasi-spherical halo is formed instead. The properties of such halos are
discussed. The rate of accretion, the radiative efficiency, and the temperature
and density near the hole are evaluated.

Affiliated with

Also associated with

No associations

Rating

Collisionless Halos Around Black Holes 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 Collisionless Halos Around Black Holes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Collisionless Halos Around Black Holes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-374209