Narrow emission line profiles in a 'quasar wind'

Details Narrow emission line profiles in a 'quasar wind' Narrow emission line profiles in a 'quasar wind'

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...302...95s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 302, March 1, 1986, p. 95-107.

Astronomy and Astrophysics

Astrophysics

12

Emission Spectra, Interstellar Matter, Quasars, Spectral Line Width, Stellar Winds, Galactic Nuclei, Molecular Clouds, Monte Carlo Method, Photoionization, Seyfert Galaxies

Scientific paper

Emission-line profiles are calculated on the basis of the recently proposed narrow emission line region model of Schiano (1986). A Monte Carlo-type calculation is used to determine emission-line profiles of an ensemble of photo-ionized interstellar clouds in a supersonic, thermal wind. These theoretical line profiles are shown to agree favorably with observations.

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