On the stability of broad line clouds in active galactic nuclei

Details On the stability of broad line clouds in active galactic nuclei On the stability of broad line clouds in active galactic nuclei

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984xue..conf..229e&link_type=abstract

In Max-Planck Inst. für Physik und Astrophysik X-Ray and UV Emission from Active Galactic Nuclei p 229-231 (SEE N85-17790 08-88)

Astronomy and Astrophysics

Astrophysics

Active Galactic Nuclei, Emission Spectra, Interstellar Gas, Line Spectra, Photoionization, Quasars, Radiation Pressure, Seyfert Galaxies

Scientific paper

The radiation pressure caused by the trapped line photons in clouds
producing the broad line emission around active galactic nuclei is
analyzed and found to be important for the stability of the clouds. It
may provide a natural explanation for the great uniformity in values of
density and ionization parameter found in quasars and Seyfert galaxies.

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