SDSS-IV MaNGA: the different quenching histories of fast and slow rotators
Do the theorised different formation mechanisms of fast and slow rotators produce an observable difference in their star formation histories? To study this we identify quenching slow rotators in the MaNGA sample by selecting those which lie below the star forming sequence and identify a sample of qu...
| Main Authors: | , , , , , , , , , , , |
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| Format: | Journal article |
| Izdano: |
Oxford University Press
2017
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