Multiple mechanisms quench passive spiral galaxies
We examine the properties of a sample of 35 nearby passive spiral galaxies in order to determine their dominant quenching mechanism(s). All five low-mass (M⋆ < 1 × 1010 M⊙) passive spiral galaxies are located in the rich Virgo cluster. This is in contrast to low-mass spiral galaxies with star for...
| Main Authors: | , , , , |
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| Format: | Article |
| Published: |
Oxford University Press
2018
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| Subjects: | |
| Online Access: | https://eprints.nottingham.ac.uk/50495/ |