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...
Main Authors: | , , , , , , , , , , , , |
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格式: | Journal article |
语言: | English |
出版: |
2007
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_version_ | 1826298860987744256 |
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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 |
format | Journal article |
id | oxford-uuid:d5b2cb15-51a9-47d2-a88b-8e43fedc1049 |
institution | University of Oxford |
language | English |
last_indexed | 2024-03-07T04:53:13Z |
publishDate | 2007 |
record_format | dspace |
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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