Interpretation of permitted-line profiles in Seyfert-galaxy and quasar spectra

Details Interpretation of permitted-line profiles in Seyfert-galaxy and quasar spectra Interpretation of permitted-line profiles in Seyfert-galaxy and quasar spectra

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pazh....5..375g&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 5, Aug. 1979, p. 375-378.) Soviet Astronomy Letters, vol. 5, July-Aug. 1979, p. 201-203

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Line Spectra, Quasars, Seyfert Galaxies, Astronomical Models, Balmer Series, Clouds, Galactic Nuclei, Interstellar Gas

Scientific paper

A model for the envelopes of Seyfert-galaxy and quasar nuclei is
developed on the hypothesis that gas clouds ejected from the nucleus are
decelerated as they travel through the intercloud gas. The Balmer-line
profiles calculated from this model are compared with the profiles
observed.

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