CO Linewidths and the Black Hole - Bulge Relationship for High Redshift QSOs

Details CO Linewidths and the Black Hole - Bulge Relationship for High Redshift QSOs CO Linewidths and the Black Hole - Bulge Relationship for High Redshift QSOs

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005rmxac..23..113m&link_type=abstract

The Ninth Texas-Mexico Conference on Astrophysics (Eds. S. Torres-Peimbert & G. MacAlpine) Revista Mexicana de Astronomía y Astr

Physics

Black Hole Physics, Galaxies: Active, Galaxies: Evolution, Quasars: General

Scientific paper

Supermassive black holes in galactic nuclei have masses MBH related to the mass and velocity dispersion σ* of the host galaxy. We examine the MBH - σ* in high redshift QSOs, deriving MBH from the broad emission-line widths and σ* from the radio CO lines. At redshifts z = 4 to 6, gigantic black holes appear to exist in relatively modest galaxies.

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