Black Hole Mass and Eddington Ratio as Drivers for the Observable Properties of Radio‐loud and Radio‐quiet QSOs

Author:

Boroson Todd A.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference24 articles.

1. Unified Models for Active Galactic Nuclei and Quasars

2. The emission-line properties of low-redshift quasi-stellar objects

3. Brandt, W. N. & Boller, T. 1999, in ASP Conf. Ser. 175, Structure and Kinematics of Quasar Broad Line Regions, ed. C. M. Gaskell, W. N. Brandt, M. Dietrich, D. Dultzin-Hacyan, & M. Eracleous (San Francisco: ASP), 265

4. On the Nature of Soft X‐Ray Weak Quasi‐stellar Objects

5. The Profiles of H beta and [O iii] lambda 5007 in Radio-loud Quasars

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