The Centre of M83
Stellar kinematics show no evidence of hidden mass concentrations at the centre of M83. We show the clearest evidence yet of an age gradient along the starburst arc and interpret the arc to have formed from orbital motion away from a starforming region in the dust lane.
| Main Authors: | , |
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| Format: | Journal article |
| Published: |
2007
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| _version_ | 1797068903502839808 |
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| author | Houghton, R Thatte, N |
| author_facet | Houghton, R Thatte, N |
| author_sort | Houghton, R |
| collection | OXFORD |
| description | Stellar kinematics show no evidence of hidden mass concentrations at the centre of M83. We show the clearest evidence yet of an age gradient along the starburst arc and interpret the arc to have formed from orbital motion away from a starforming region in the dust lane. |
| first_indexed | 2024-03-06T22:16:42Z |
| format | Journal article |
| id | oxford-uuid:539c2b81-8164-4cb5-976d-394baf07c042 |
| institution | University of Oxford |
| last_indexed | 2024-03-06T22:16:42Z |
| publishDate | 2007 |
| record_format | dspace |
| spelling | oxford-uuid:539c2b81-8164-4cb5-976d-394baf07c0422022-03-26T16:32:48ZThe Centre of M83Journal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:539c2b81-8164-4cb5-976d-394baf07c042Symplectic Elements at Oxford2007Houghton, RThatte, NStellar kinematics show no evidence of hidden mass concentrations at the centre of M83. We show the clearest evidence yet of an age gradient along the starburst arc and interpret the arc to have formed from orbital motion away from a starforming region in the dust lane. |
| spellingShingle | Houghton, R Thatte, N The Centre of M83 |
| title | The Centre of M83 |
| title_full | The Centre of M83 |
| title_fullStr | The Centre of M83 |
| title_full_unstemmed | The Centre of M83 |
| title_short | The Centre of M83 |
| title_sort | centre of m83 |
| work_keys_str_mv | AT houghtonr thecentreofm83 AT thatten thecentreofm83 AT houghtonr centreofm83 AT thatten centreofm83 |