MEGA-MASERS AND GALAXIES

By K. Lo. 2005

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THE MEGAMASER COSMOLOGY PROJECT. III. ACCURATE MASSES OF SEVEN SUPERMASSIVE BLACK HOLES IN ACTIVE GALAXIES WITH CIRCUMNUCLEAR MEGAMASER DISKS (2010, background): “The Compton thick nature of these AGNs is a problem because the intrinsic radiation is mostly suppressed and the X-ray spectrum is dominated by the reflected or scattered components.”
The dusty torus in the Circinus galaxy: a dense disk and the torus funnel (2013, background): “This contradicts the parsec-sized, equatorially extended emission of our disk-like component as well as the requirements for the pumping of the disk masers, which require a direct line of sight to the central engine (Greenhill et al. 2003; Lo 2005).”
The Hubble Constant (2010, background): “J. 417:553 Lemâıtre(1927)Lemâıtre, G. 1927, Annales de la Societe Scientifique de Bruxelles, 47:49 Lo(2005)Lo KY. 2005.”
PRECISE BLACK HOLE MASSES FROM MEGAMASER DISKS: BLACK HOLE–BULGE RELATIONS AT LOW MASS (2010, background): “The cleanest and best-studied megamaser galaxy is the nearby Seyfert galaxy NGC 4258 (e.g., Nakai et al. 1993; 1 Greenhill et al. 1995; Miyoshi et al. 1995; Herrnstein et al. 1996, and for a complete literature review see Lo 2005).”