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SINFONI's take on Star Formation, Molecular Gas, and Black Hole Masses in AGN

R. Davies·R. Genzel·L. Tacconi·F. Muller Sanchez·J. Thomas·S. Friedrich
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Abstract

We present some preliminary (half-way) results on our adaptive optics spectroscopic survey of AGN at spatial scales down to 0.085arcsec. Most of the data were obtained with SINFONI which provides integral field capability at a spectral resolution of R~4000. The themes on which we focus in this contribution are: star formation around the AGN, the properties of the molecular gas and its relation to the torus, and the mass of the black hole.

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R. Davies, R. Genzel, L. Tacconi, F. Muller Sanchez, J. Thomas, S. Friedrich. 2006-01-19. SINFONI's take on Star Formation, Molecular Gas, and Black Hole Masses in AGN. https://doi.org/10.1007/978-3-540-73491-8_41

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