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| Morphological features | Kinematics feat. | Differ. in | M/LB | Other | INTERACTION | ||||||
| Galaxy | Plume | Tail | Merger | TDGs | H II gas | H I gas | abundances | ratios | features | DEGREE | |
| HCG 31 ACa | X | X | X | X | X | X | X | X | X | VERY HIGH | |
| Mkn 1087 | - | X | - | X | X | ... | X | - | - | HIGH | |
| Haro 15 | ? | - | X | ? | X | ... | X | - | - | VERY HIGH | |
| Mkn 1199a | X | - | X | - | X | ... | X | X | X | VERY HIGH | |
| Mkn 5 | - | - | - | - | - | ... | ? | X | X | LOW | |
| IRAS 08208+2816 | - | X | ? | ? | X | ... | X | - | - | VERY HIGH | |
| IRAS 08339+6517a | X | - | - | ? | X | X | - | - | - | HIGH | |
| POX 4 | X | - | - | ? | X | X | - | - | X | HIGH | |
| UM 420 | - | X | ? | - | ? | ... | - | - | - | VERY HIGH | |
| SBS 0926+606 A | X | - | X | - | X | ... | - | - | - | VERY HIGH | |
| SBS 0926+606 B | X | X | ? | X | ... | - | - | - | HIGH | ||
| SBS 0948+532 | - | X | - | - | ? | ... | - | X | - | PROBABLE | |
| SBS 1054+365 | - | - | - | ? | X | ... | - | X | X | LOW | |
| SBS 1211+540 | X | - | ? | - | X | ... | - | - | - | PROBABLE | |
| SBS 1319+579 | - | - | ? | - | X | ... | ? | X | X | PROBABLE | |
| SBS 1415+437 | - | - | - | - | ? | ... | - | - | - | LOW | |
| III Zw 107 | X | - | ? | - | X | ... | ? | X | - | HIGH | |
| Tol 9 | X | - | - | - | X | X | - | X | X | HIGH | |
| Tol 1457-262 | X | - | X | X | X | ... | X | - | - | VERY HIGH | |
| Arp 252a | X | X | - | X | X | ... | X | - | - | VERY HIGH | |
| NGC 5253 | - | - | - | - | X | X | X | X | X | PROBABLEb | |
Notes. (a) Some
interaction features in this galaxy were previously reported by other
authors.
(b) The chemical
differences and the kinematics features can be explained by other
reasons. See López-Sánchez et al. (2007, 2010a).
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