z-logo
open-access-imgOpen Access
Physical conditions in thin laminar-convective accretion flows
Author(s) -
Konstantin Malanchev,
К. А. Постнов,
Н. И. Шакура
Publication year - 2019
Publication title -
journal of physics. conference series
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.21
H-Index - 85
eISSN - 1742-6596
pISSN - 1742-6588
DOI - 10.1088/1742-6596/1390/1/012085
Subject(s) - laminar flow , convection , convective flow , mechanics , accretion (finance) , flow (mathematics) , materials science , astrophysics , physics
The physical conditions of convection appearance in laminar accretion flows with microscopic transport coefficients are examined. Hot sparse ionised flow with periods below an hour found to be optically thin and have convective layer. Cold sparse molecular flow with period about a year found to be optically thin too and are fully convective. Ranges of temperature, density and period of optically thick laminar accretion flow are shown.

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here