On gaseous disks in Seyfert 1 nuclei

Details On gaseous disks in Seyfert 1 nuclei On gaseous disks in Seyfert 1 nuclei

Nov 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...262..554a&link_type=abstract

Astrophysical Journal, Part 1, vol. 262, Nov. 15, 1982, p. 554, 555.

Astronomy and Astrophysics

Astrophysics

Cosmic Gases, Galactic Nuclei, Galactic Structure, Rotating Disks, Seyfert Galaxies, Angular Velocity, Orthogonality

Scientific paper

Implications of the suggestion that the broad-line component of a
Seyfert 1 nucleus arises in a rotating disk whose plane is orthogonal to
that of the parent galaxy are considered. Observed line widths would be
expected to decrease, and their dispersion about the mean relation to
increase, with increasing inclination of the parent galaxy

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