A unified accretion model reveals an effectively optically thin, radiation-pressure-supported flow between the standard thin disk and slim disk, producing a multi-color Wien spectrum and constraining viscosity to alpha ~ 0.03.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.HE 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
The effectively optically thin accretion flow and its implication in supermassive black holes
A unified accretion model reveals an effectively optically thin, radiation-pressure-supported flow between the standard thin disk and slim disk, producing a multi-color Wien spectrum and constraining viscosity to alpha ~ 0.03.