Dynamics of the Nuclear Outflow in NGC 1068

Details Dynamics of the Nuclear Outflow in NGC 1068 Dynamics of the Nuclear Outflow in NGC 1068

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ap%26ss.248..207k&link_type=abstract

Astrophysics and Space Science, Volume 248, Issue 1-2, pp. 207-215

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

A short survey is presented of dynamical (and thermodynamical) issues relevant to outflows in Seyfert galaxies like NGC 1068. Numerical simulations incorporating both realistic radiative heating and cooling, and angular momentum, show that the fraction of injected gas which escapes in a wind is very sensitive to both the injection pressure and the gas's angular momentum. Radiation pressure acting through a variety of atomic opacity processes may also be important.

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