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Integral Field Spectroscopy of z ~ 0.1 QSO Host Galaxies

Published online by Cambridge University Press:  03 June 2010

Dading Nugroho ,
Knud Jahnke ,
Bernd Husemann ,
Katherine Inskip ,
Sebastian F. Sánchez  and
Lutz Wisotzki
Dading Nugroho
Affiliation:
MPIA, Königstuhl 17, D-69117 Heidelberg, Germany Email: [email protected]
Knud Jahnke
Affiliation:
MPIA, Königstuhl 17, D-69117 Heidelberg, Germany Email: [email protected]
Bernd Husemann
Affiliation:
Astrophysikalisches Institut Potsdam, An der Sternwarte 16, D-14482 Potsdam, Germany
Katherine Inskip
Affiliation:
MPIA, Königstuhl 17, D-69117 Heidelberg, Germany Email: [email protected]
Sebastian F. Sánchez
Affiliation:
CAHA, C/ Jesús Durbán Remón, 2-2, 04004 Almeria, Spain
Lutz Wisotzki
Affiliation:
Astrophysikalisches Institut Potsdam, An der Sternwarte 16, D-14482 Potsdam, Germany
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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.

Keywords

galaxies: activegalaxies: quasarsgalaxies: nucleigalaxies: ISM
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S267: Co-Evolution of Central Black Holes and Galaxies , August 2009 , pp. 334
Copyright
Copyright © International Astronomical Union 2010

References

Jahnke, K., Kuhlbrodt, B., & Wisotzki, L. 2004, MNRAS, 352, 399CrossRefGoogle Scholar
Husemann, B., Wisotzki, L., Sánchez, S. F., & Jahnke, K. 2008, A&A, 488, 145Google Scholar