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Table 2.
Percentage of galaxies with kinematically confirmed outflows in the literature depending on their morphological classification of the Hα nuclear emission (see Sect. 5.1 and Appendix A for the comments on individual targets).
Morphological class | Kinematical outflows | Targets |
---|---|---|
Core-halo | 50% | 8 (out of 16) |
Disky | 31% | 4 (out of 13) |
Dusty | 66% | 4 (out of 6) |
Bubble | 48% | 10 (out of 21) |
Unclear | 75% | 3 (out of 4) |
All classes | 48% | 29 (out of 60) |
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