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The Centre of M83

Abstract:
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.

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Publisher copy:
10.1017/S1743921308017997

Authors


More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author


Journal:
Proceedings of the International Astronomical Union More from this journal
Volume:
3
Issue:
S245
Publication date:
2007-10-09
DOI:
EISSN:
1743-9221
ISSN:
1743-9213


Keywords:
Pubs id:
pubs:221886
UUID:
uuid:539c2b81-8164-4cb5-976d-394baf07c042
Local pid:
pubs:221886
Source identifiers:
221886
Deposit date:
2013-11-17

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