Published in
Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S245(3), p. 215-218, 2007
DOI: 10.1017/s1743921308017687
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Supermassive black holes from OASIS and SAURON integral-field kinematics
Journal article published in 2007 by
Michele Cappellari 
,
R. Bacon,
Roger L. Davies,
P. T. de Zeeuw,
Eric Emsellem,
Jesús Falcón-Barroso,
Davor Krajnović,
Harald Kuntschner,
Richard M. McDermid,
Reynier F. Peletier ,
Marc Sarzi,
Remco C. E. van den Bosch,
Glenn van de Ven
,
R. Bacon,
Roger L. Davies,
P. T. de Zeeuw,
Eric Emsellem,
Jesús Falcón-Barroso,
Davor Krajnović,
Harald Kuntschner,
Richard M. McDermid,
Reynier F. Peletier ,
Marc Sarzi,
Remco C. E. van den Bosch,
Glenn van de Ven
This paper was not found in any repository, but could be made available legally by the author.
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Abstract
AbstractSupermassive 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.
