Hostname: page-component-6bf8c574d5-2jptb Total loading time: 0 Render date: 2025-02-18T00:08:03.306Z Has data issue: false hasContentIssue false
  • English
  • Français

No Evolution in the MBH–M*,total Relation Over the Last 9 Gyrs

Published online by Cambridge University Press:  03 June 2010

Knud Jahnke ,
Mauricio Cisternas  and
Katherine J. Inskip
Knud Jahnke
Affiliation:
MPIA, Königstuhl 17, D-69126 Heidelberg, Germany Email: [email protected]
Mauricio Cisternas
Affiliation:
MPIA, Königstuhl 17, D-69126 Heidelberg, Germany Email: [email protected]
Katherine J. Inskip
Affiliation:
MPIA, Königstuhl 17, D-69126 Heidelberg, Germany Email: [email protected]
Rights & Permissions [Opens in a new window]

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We investigate 10 QSO host galaxies at 1<z<2 in the COSMOS field (Scoville et al. 2007), observed with the HST in both ACS/WFC I-band and NICMOS/NIC3 H-band. We find that our galaxies with mean z = 1.4 follow the local MBH–Mbulge relation exactly – however, not with an explicit bulge mass, but with their total stellar mass.

Keywords

galaxies: activequasars: generalgalaxies: evolution
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. 206
Copyright
Copyright © International Astronomical Union 2010

References

Häring, N. & Rix, H.-W. 2004, ApJ, 604, L89CrossRefGoogle Scholar
Ilbert, O., et al. 2009, submitted to ApJ [arXiv:0903.0102]Google Scholar
Jahnke, K., et al. 2009, ApJ, 706, L215CrossRefGoogle Scholar
Merloni, A., et al. 2009, ApJ, in press [arXiv:0910.4970]Google Scholar
Trump, J. R., et al. 2009, ApJ, 700, 49CrossRefGoogle Scholar
Scoville, N., et al. 2007, ApJS, 172, 38CrossRefGoogle Scholar