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Supermassive black holes from OASIS and SAURON integral-field kinematics

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. © 2008 Copyright International Astronomical Union 2008.

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Publisher copy:
10.1017/S1743921308017687

Authors


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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
Expand authors...
Journal:
Proceedings of the International Astronomical Union
Volume:
3
Issue:
S245
Pages:
215-218
Publication date:
2007-07-01
DOI:
EISSN:
1743-9221
ISSN:
1743-9213
Source identifiers:
190072
Language:
English
Keywords:
Pubs id:
pubs:190072
UUID:
uuid:d5b2cb15-51a9-47d2-a88b-8e43fedc1049
Local pid:
pubs:190072
Deposit date:
2012-12-19

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