What can we learn on the BLR from the smallest AGN? Or, how do the BLR properties change with luminosity, and what is it telling us? Specifically The BLR.
On the geometry of broad emission region in quasars Roberto Decarli Turin - May, 20 th, 2008 Università degli Studi dell’Insubria Dipartimento di Fisica.
1 Black Hole Masses from Reverberation Mapping Bradley M. Peterson The Ohio State University Collaborators: M. Bentz, S. Collin, K. Dasyra, K. Denney,
Dark matter and black holes over cosmic time TOMMASO TREU.
Black Hole Press Kit
The Michigan/Magellan Fiber System (M2FS): An MRI Instrument Development Proposal to NSF.
The Evolution of Quasars and Massive Black Holes “Quasar Hosts and the Black Hole-Spheroid Connection”: Dunlop 2004 “The Evolution of Quasars”: Osmer 2004.
Biases in Virial Black Hole Masses: an SDSS Perspective
On the role of density and Eddington ratio in the correlation space of NLS1 galaxies
Active Galactic Nuclei: Progress and Problems Martin Gaskell Astronomy Department, University of Texas, Austin, TX 78712-0259, USA [email protected].
Super-massive Black Holes of Quasars at World ’ s End
Introduction Highly accreting AGN on the M-sigma relation Flares from tidally disrupted stars