Table 3.
Numbers and fractions of galaxies, with the given kinematic class having shells, streams, tails, or satellite planes.
| Type | All | Shells | Streams | Tails | Planes |
|---|---|---|---|---|---|
| RR | 286 | 2 | 26 | 8 | 63 |
| 1 ± 1% | 9 ± 2% | 3 ± 1% | 22 ± 3% | ||
| NR | 108 | 10 | 16 | 2 | 19 |
| 9 ± 3% | 15 ± 4% | 2 ± 2% | 18 ± 5% | ||
| KDC | 26 | 1 | 6 | 2 | 1 |
| 4 ± 4% | 23 ± 10% | 8 ± 6% | 4 ± 4% | ||
| PR | 16 | 3 | 3 | 2 | 2 |
| 19 ± 11% | 19 ± 11% | 13 ± 9% | 13 ± 9% |
Notes. Only the subset of our full sample that was kinematically classified by Schulze et al. (2018) was considered for the numbers and fractions. This subsample comprises 436 galaxies. The kinematic classes include regular rotators (RR), nonrotators (NR), KDCs, and prolate rotators (PR).
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