Nuclear Star Clusters and Black Holes
We summarize the recent results of our survey of the nearest nuclear star clusters. The purpose of the survey is to understand nuclear star cluster formation mechanisms and constrain the presence of black holes using adaptive optics assisted integral field spectroscopy, optical spectroscopy, and HST...
| Main Authors: | , , , , , , , , , , |
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| Format: | Conference item |
| Published: |
2010
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| _version_ | 1797064401550835712 |
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| author | Seth, A Cappellari, M Neumayer, N Caldwell, N Bastian, N Olsen, K Blum, R Debattista, V McDermid, R Puzia, T Stephens, A |
| author_facet | Seth, A Cappellari, M Neumayer, N Caldwell, N Bastian, N Olsen, K Blum, R Debattista, V McDermid, R Puzia, T Stephens, A |
| author_sort | Seth, A |
| collection | OXFORD |
| description | We summarize the recent results of our survey of the nearest nuclear star clusters. The purpose of the survey is to understand nuclear star cluster formation mechanisms and constrain the presence of black holes using adaptive optics assisted integral field spectroscopy, optical spectroscopy, and HST imaging in 13 galaxies within 5 Mpc. We discuss the formation history of the nuclear star cluster and possible detection of an intermediate mass BH in NGC 404, the nearest S0 galaxy. © 2010 American Institute of Physics. |
| first_indexed | 2024-03-06T21:13:46Z |
| format | Conference item |
| id | oxford-uuid:3f10e098-a03d-41dc-ba9d-058f03267ba3 |
| institution | University of Oxford |
| last_indexed | 2024-03-06T21:13:46Z |
| publishDate | 2010 |
| record_format | dspace |
| spelling | oxford-uuid:3f10e098-a03d-41dc-ba9d-058f03267ba32022-03-26T14:29:39ZNuclear Star Clusters and Black HolesConference itemhttp://purl.org/coar/resource_type/c_5794uuid:3f10e098-a03d-41dc-ba9d-058f03267ba3Symplectic Elements at Oxford2010Seth, ACappellari, MNeumayer, NCaldwell, NBastian, NOlsen, KBlum, RDebattista, VMcDermid, RPuzia, TStephens, AWe summarize the recent results of our survey of the nearest nuclear star clusters. The purpose of the survey is to understand nuclear star cluster formation mechanisms and constrain the presence of black holes using adaptive optics assisted integral field spectroscopy, optical spectroscopy, and HST imaging in 13 galaxies within 5 Mpc. We discuss the formation history of the nuclear star cluster and possible detection of an intermediate mass BH in NGC 404, the nearest S0 galaxy. © 2010 American Institute of Physics. |
| spellingShingle | Seth, A Cappellari, M Neumayer, N Caldwell, N Bastian, N Olsen, K Blum, R Debattista, V McDermid, R Puzia, T Stephens, A Nuclear Star Clusters and Black Holes |
| title | Nuclear Star Clusters and Black Holes |
| title_full | Nuclear Star Clusters and Black Holes |
| title_fullStr | Nuclear Star Clusters and Black Holes |
| title_full_unstemmed | Nuclear Star Clusters and Black Holes |
| title_short | Nuclear Star Clusters and Black Holes |
| title_sort | nuclear star clusters and black holes |
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