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Supermassive black holes from OASIS and SAURON integral-field kinematics
Published online by Cambridge University Press: 01 July 2007
Abstract
Supermassive black holes are a key element in our understanding of how galaxies form. Most of the progress in this very active field of research is based on just ~30 determination of black hole masses, accumulated over the past decade. We illustrate how integral-field spectroscopy, and in particular our OASIS modeling effort can help improve the current situation.
Keywords
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 3 , Symposium S245: Formation and Evolution of Galaxy Bulges , July 2007 , pp. 215 - 218
- Copyright
- Copyright © International Astronomical Union 2008
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