Resolving the Dynamical Mass of a z ~ 1.3 Quasi-stellar Object Host Galaxy Using SINFONI and Laser Guide Star Assisted Adaptive Optics

Recent studies of the tight scaling relations between the masses of supermassive black holes (BHs) and their host galaxies have suggested that in the past BHs constituted a larger fraction of their host galaxies' mass. However, these arguments are limited by selection effects and difficulties i...

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Veröffentlicht in:	The Astrophysical journal 2011-10, Vol.739 (2), p.90-jQuery1323903136161='48'
Hauptverfasser:	Inskip, K. J, Jahnke, K, Rix, H.-W, van de Ven, G
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Earth, ocean, space Exact sciences and technology
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