Statistical study of AGN's. I - Line widths of C IV and H-beta versus optical luminosity

Details Statistical study of AGN's. I - Line widths of C IV and H-beta versus optical luminosity Statistical study of AGN's. I - Line widths of C IV and H-beta versus optical luminosity

Nov 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...152..282j&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 152, no. 2, Nov. 1985, p. 282-290.

Astronomy and Astrophysics

Astrophysics

50

Active Galactic Nuclei, Carbon, H Beta Line, Luminous Intensity, Quasars, Spectral Line Width, Statistical Analysis, Radio Galaxies, Seyfert Galaxies, Ultraviolet Spectra

Scientific paper

Results are presented of a statistical analysis of H-beta and C IV 1550 line widths and optical luminosities for a large sample of Seyfert 1 nuclei, quasars, and broad line radiogalaxies. Physical properties of the broad line radiogalaxies, including the accretion process itself in the framework of gravitational models, are deduced. For high-luminosity quasars, the gravitational mode used may be questionable in view of the very large masses involved.

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