BALMER EMISSION LINE PROFILES AND COMPLEX PROPERTIES OF BROAD-LINE REGIONS IN ACTIVE GALACTIC NUCLEI
Authors:
- G. La MuraGMG. La Mura
- F. Di MilleFMF. Di Mille
- S. CiroiSCS. Ciroi
- L. Č. PopovićLPL. Č. Popović
- P. RafanelliPRP. Rafanelli
- 9 March 2009
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 693 (2) , 1437-1448
Abstract
No abstract availableAll Related Versions
This publication has 69 references indexed in Scilit:
- The Sixth Data Release of the Sloan Digital Sky SurveyThe Astrophysical Journal Supplement Series, 2008
- The Radius‐Luminosity Relationship for Active Galactic Nuclei: The Effect of Host‐Galaxy Starlight on Luminosity MeasurementsThe Astrophysical Journal, 2006
- Exploring Narrow-Line Seyfert 1 Galaxies through the Physical Properties of Their HostsThe Astronomical Journal, 2004
- Rotation Curve Measurement using Cross‐Correlation1Publications of the Astronomical Society of the Pacific, 2000
- Are AGN broad emission lines formed by discrete clouds? Analysis of Keck high-resolution spectroscopy of NGC 4151Monthly Notices of the Royal Astronomical Society, 1998
- Keck high-resolution spectroscopy of Mrk 335: constraints on the number of emitting clouds in the broad-line regionMonthly Notices of the Royal Astronomical Society, 1997
- The relationship between infrared, optical, and ultraviolet extinctionThe Astrophysical Journal, 1989
- Reverberation mapping of the emission line regions of Seyfert galaxies and quasarsThe Astrophysical Journal, 1982
- The dynamics of the broad-line-emitting regions of active galactic nuclei and quasars. II - Discrete cloud models and line profile asymmetriesThe Astrophysical Journal, 1981
- The dynamics of the broad-line-emitting regions of active galactic nuclei and quasars. I - Broad-line profilesThe Astrophysical Journal, 1980