Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990azh....67..230z&link_type=abstract
Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 67, Mar.-Apr. 1990, p. 230-240. In Russian.
Astronomy and Astrophysics
Astronomy
Active Galactic Nuclei, Cosmic Gases, Galactic Radiation, Gas Dynamics, Equations Of Motion, Flow Velocity, Gravitational Effects, Radiation Pressure
Scientific paper
The hydrodynamic structure of the wind flowing out from an active galactic nucleus is calculated. It is shown that, in the range of broad line formation, the velocity of the wind reaches a value that is not greater than twice that at the inner boundary. The motion of emission clouds in the outflow envelope is examined, and conditions for the almost total entrainment of the cloud by the wind are established.
Hadrava Petr
Zentsova Anna S.
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