Spectroscopic Study of C IV lambda 1549 and its Relation with Optical Parameters in Active Galactic Nuclei

Details Spectroscopic Study of C IV lambda 1549 and its Relation with Optical Parameters in Active Galactic Nuclei Spectroscopic Study of C IV lambda 1549 and its Relation with Optical Parameters in Active Galactic Nuclei

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008rmxac..32..106n&link_type=abstract

The Nuclear Region, Host Galaxy and Environment of Active Galaxies (Eds. Erika Benítez, Irene Cruz-González, & Yair Krongold) Re

Astronomy and Astrophysics

Astronomy

Quasars: General, Quasars: Emission Lines, Quasars: Line Profiles

Scientific paper

We explore the relation between optical and UV parameters for all known
types of broad line emitting AGN using our 4D Eigenvector 1 parameter
space, in an attempt of a spectroscopic unification scheme. Black hole
masses computed from FWHM(C IV lambda 1549_{BC}) indicate that the C IV
lambda 1549 width is a poor virial estimator.

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