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Integral field spectroscopy of QSO host galaxies

  • We describe a project to study the state of the ISM in similar to20 low redshift (z < 0.3) QSO host galaxies observed with the PMAS integral field spectrograph. We describe the development of the method to access the stellar and gas components of the spectrum without the strong nuclear emission, in order to access the host galaxy properties in the central region. It shows that integral field spectroscopy promises to be very efficient in studying the gas distribution and its velocity field, and also the spatially resolved stellar population in the host galaxies of luminous AGN

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Author details:Knud Jahnke, Lutz WisotzkiORCiDGND, Sebastian F. Sanchez, Lise Bech ChristensenORCiD, Thomas BeckerGND, A. Kelz, Martin M. RothORCiDGND
Publication type:Article
Language:English
Year of first publication:2004
Publication year:2004
Release date:2017/03/24
Source:Astronomische Nachrichten. - 325 (2004), 2, S. 128 - 131
Organizational units:Mathematisch-Naturwissenschaftliche Fakultät / Institut für Physik und Astronomie
Peer review:Referiert
Institution name at the time of the publication:Mathematisch-Naturwissenschaftliche Fakultät / Institut für Physik
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