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...
| 主要な著者: | , , , , , , , , , , , |
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| フォーマット: | Journal article |
| 出版事項: |
Oxford University Press
2017
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