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An Hα Dynamical Mass for HE 0047–1756

Published online by Cambridge University Press:  03 June 2010

K. J. Inskip ,
K. Jahnke ,
H.-W. Rix  and
C. Y. Peng
K. J. Inskip
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany Email: inskip@mpia.de, jahnke@mpia.de, rix@mpia.de
K. Jahnke
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany Email: inskip@mpia.de, jahnke@mpia.de, rix@mpia.de
H.-W. Rix
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany Email: inskip@mpia.de, jahnke@mpia.de, rix@mpia.de
C. Y. Peng
Affiliation:
Herzberg Institute of Astrophysics, National Research Council of Canada, 5071 West Saanich Rd., Victoria, BC V9E 2E7, Canada Email: cyp@nrc-cnrc.gc.ca
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Abstract

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We derive Mbulge for HE 0047–1756 via Hα gas dynamics. The resulting large value of MBH/Mbulge may imply evolution in the correlation at high redshifts.

Keywords

galaxies: activegalaxies: evolutionquasars: individual (HE 0047–1756)
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. 205
Copyright
Copyright © International Astronomical Union 2010

References

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