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: http://xray.sai.msu.ru/sciwork/archive/68/eannot1.html
Дата изменения: Mon Oct 16 15:48:52 2000
Дата индексирования: Tue Oct 2 12:11:02 2012
Кодировка:
We propose a simultaneous solution
scheme for coupled inflow-outflow systems in order to probe the
hydrodynamical
origin of accretion-powered astrophysical outflows from galactic and
extragalactic sources harbouring accreting massive compact objects. By
self-consistent
combination of accretion and wind solutions, we compute the mass outflow
rate Rdot m
in terms of accretion parameters and study the dependence
of Rdot m on various physical parameters governing the
flow. Unlike the self-similar
solutions present in the literature, our non-self-similar model
points out the exact location
from where these outflows are launched.