Advection-Dominated Accretion Disks: Geometrically Slim or Thick?
classification
🌌 astro-ph.HE
keywords
disksaccretionadvection-dominatedgeometricallyslimthickadvectiveangle
read the original abstract
We revisit the vertical structure of black hole accretion disks in spherical coordinates. By comparing the advective cooling with the viscous heating, we show that advection-dominated disks are geometrically thick, i.e., with the half-opening angle > 2\pi/5, rather than slim as supposed previously in the literature.
This paper has not been read by Pith yet.
Forward citations
Cited by 1 Pith paper
-
Little Red Dots as Supermassive Analogs of SS 433
LRDs are interpreted as high-inclination hyper-Eddington accreting SMBHs analogous to SS 433, with V-shaped SEDs, X-ray weakness, and Balmer breaks emerging from disk self-shielding geometry.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.