The influence of rotating wind in supercritical accretion disk with radiation pressure

We solved one-dimensional hydrodynamic (HD) equations of the slim disks in the presence of the wind and in cylindrical coordinates using self-similar solution. We considered power-law function of for mass loss rate due to wind. Then, we considered mass loss, angular-momentum loss and energy loss in...

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Bibliographic Details
Main Authors: F Z Zeratgari, E Delkhani, Sh Abbassi
Format: Article
Language:English
Published: Isfahan University of Technology 2018-02-01
Series:Iranian Journal of Physics Research
Subjects:
Online Access:http://ijpr.iut.ac.ir/browse.php?a_code=A-10-425-1&slc_lang=en&sid=1

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