Accretion Disks Around Black Holes: Twenty Five Years Later
classification
🌌 astro-ph
gr-qc
keywords
blackdisksaccretionaroundfiveholestwentyyears
read the original abstract
We study the progress of the theory of accretion disks around black holes in last twenty five years and explain why advective disks are the best bet in explaining varied stationary and non-stationary observations from black hole candidates. We show also that the recently proposed advection dominated flows are incorrect.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.