Supermassive black holes from OASIS and SAURON integral-field kinematics

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...

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Main Authors: Cappellari, M, Bacon, R, Davies, R, De Zeeuw, P, Emsellem, E, Falcón-Barroso, J, Krajnović, D, Kuntschner, H, McDermid, R, Peletier, R, Sarzi, M, Van Den Bosch, R, Van De Ven, G
格式: Journal article
语言:English
出版: 2007
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author Cappellari, M
Bacon, R
Davies, R
De Zeeuw, P
Emsellem, E
Falcón-Barroso, J
Krajnović, D
Kuntschner, H
McDermid, R
Peletier, R
Sarzi, M
Van Den Bosch, R
Van De Ven, G
author_facet Cappellari, M
Bacon, R
Davies, R
De Zeeuw, P
Emsellem, E
Falcón-Barroso, J
Krajnović, D
Kuntschner, H
McDermid, R
Peletier, R
Sarzi, M
Van Den Bosch, R
Van De Ven, G
author_sort Cappellari, M
collection OXFORD
description 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.
first_indexed 2024-03-07T04:53:13Z
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spelling oxford-uuid:d5b2cb15-51a9-47d2-a88b-8e43fedc10492022-03-27T08:27:52ZSupermassive black holes from OASIS and SAURON integral-field kinematicsJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:d5b2cb15-51a9-47d2-a88b-8e43fedc1049EnglishSymplectic Elements at Oxford2007Cappellari, MBacon, RDavies, RDe Zeeuw, PEmsellem, EFalcón-Barroso, JKrajnović, DKuntschner, HMcDermid, RPeletier, RSarzi, MVan Den Bosch, RVan De Ven, GSupermassive 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.
spellingShingle Cappellari, M
Bacon, R
Davies, R
De Zeeuw, P
Emsellem, E
Falcón-Barroso, J
Krajnović, D
Kuntschner, H
McDermid, R
Peletier, R
Sarzi, M
Van Den Bosch, R
Van De Ven, G
Supermassive black holes from OASIS and SAURON integral-field kinematics
title Supermassive black holes from OASIS and SAURON integral-field kinematics
title_full Supermassive black holes from OASIS and SAURON integral-field kinematics
title_fullStr Supermassive black holes from OASIS and SAURON integral-field kinematics
title_full_unstemmed Supermassive black holes from OASIS and SAURON integral-field kinematics
title_short Supermassive black holes from OASIS and SAURON integral-field kinematics
title_sort supermassive black holes from oasis and sauron integral field kinematics
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