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

Astronomy and Astrophysics – Astronomy

Scientific paper

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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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