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Table 2.
Fraction of quenched galaxies across morphologies in different environments.
| Galaxy morphology | Control sample | Isolated CGs | Non-isolated CGs |
|---|---|---|---|
| All galaxies | 0.42 ± 0.01 | 0.52 ± 0.04 | 0.71 ± 0.02 |
| ETGs | 0.87 ± 0.02 | 0.77 ± 0.05 | 0.91 ± 0.02 |
| Transition galaxies | 0.53 ± 0.03 | 0.39 ± 0.10 | 0.67 ± 0.08 |
| LTGs | 0.06 ± 0.01 | 0.05 ± 0.03 | 0.12 ± 0.04 |
Notes. Fraction of quenched galaxies for different galaxy morphologies in the control sample, isolated CGs, and non-isolated CGs. The criterion proposed by Wetzel et al. (2013) (log(sSFR) ≤ −11) is used to determine if a galaxy is quenched.
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