TY - JOUR
T1 - Supermassive black holes from OASIS and SAURON integral-field kinematics
AU - Cappellari, Michele
AU - Bacon, R.
AU - Davies, Roger L.
AU - De Zeeuw, P. T.
AU - Emsellem, Eric
AU - Falcón-Barroso, Jesús
AU - Krajnović, Davor
AU - Kuntschner, Harald
AU - McDermid, Richard M.
AU - Peletier, Reynier F.
AU - Sarzi, Marc
AU - Van Den Bosch, Remco C E
AU - Van De Ven, Glenn
PY - 2007/7
Y1 - 2007/7
N2 - 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.
AB - 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.
KW - Black hole physics
KW - Galaxies: elliptical and lenticular
KW - Galaxies: kinematics and dynamics
KW - Galaxies: nuclei
UR - http://www.scopus.com/inward/record.url?scp=46749119512&partnerID=8YFLogxK
U2 - 10.1017/S1743921308017687
DO - 10.1017/S1743921308017687
M3 - Article
AN - SCOPUS:46749119512
SN - 1743-9213
VL - 3
SP - 215
EP - 218
JO - Proceedings of the International Astronomical Union
JF - Proceedings of the International Astronomical Union
IS - S245
ER -