Gaseous disks in Seyfert 1 nuclei
Journal Article
·
· Astrophys. J.; (United States)
We consider some 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. Observed line widths would be expected to decrease, and their dispersion about the mean relation to increase, with increasing inclination of the parent galaxy.
- Research Organization:
- Department of Astronomy, New Mexico State University
- OSTI ID:
- 5577271
- Journal Information:
- Astrophys. J.; (United States), Vol. 262:2
- Country of Publication:
- United States
- Language:
- English
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