SINFONI's take on star formation, molecular gas, and black hole masses in AGN
We present some preliminary (half-way) results on our adaptive optics spectroscopic survey of AGN at spatial scales down to 0.085″. 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. © 2007 Springer-Verlag Berlin Heidelberg.
ESO Astrophysics Symposia
Davies, R., Genzel, R., Tacconi, L., Müller Sanchez, F., Thomas, J., & Friedrich, S. (2007). SINFONI's take on star formation, molecular gas, and black hole masses in AGN. ESO Astrophysics Symposia, 2007, 259-263. https://doi.org/10.1007/978-3-540-73491-8_41