Nuclear Winds and Line Emission in Active Galaxies

Details Nuclear Winds and Line Emission in Active Galaxies Nuclear Winds and Line Emission in Active Galaxies

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aas...181.7104s&link_type=abstract

American Astronomical Society, 181st AAS Meeting, #71.04; Bulletin of the American Astronomical Society, Vol. 24, p.1234

Astronomy and Astrophysics

Astronomy

Scientific paper

The relationship between line emission and nuclear winds in active galaxies is discussed. Narrow-line clouds, as well as broad-line and broad-absorption line clouds, can be accelerated to their inferred velocities with only a weak dependence on parameters. However the clouds must survive longer than linear instability growth rates would indicate. This poster focuses on analysis of the line emission of individual galaxies in the context of nuclear winds.

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