Integral Field Spectroscopy of z ~ 0.1 QSO Host Galaxies

Details Integral Field Spectroscopy of z ~ 0.1 QSO Host Galaxies Integral Field Spectroscopy of z ~ 0.1 QSO Host Galaxies

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010iaus..267..334n&link_type=abstract

Co-Evolution of Central Black Holes and Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Volume 267

Astronomy and Astrophysics

Astronomy

Galaxies: Active, Galaxies: Quasars, Galaxies: Nuclei, Galaxies: Ism

Scientific paper

We observed a volume-limited sample of 19 luminous type 1 QSO host galaxies at MV ~ -23 mag and redshift 0.06 < z < 0.2 (Jahnke et al. 2004) using the VLT/VIMOS Integral Field Spectrograph. After removal of the QSO contribution (using the method of Husemann et al. 2008), we construct 2D intensity maps and gas velocity fields of the host galaxies in the Hα and [O iii] emission lines. Two representative cases are shown in Figure 1.

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