Table 3.
IR fractions.
| No. | Galaxy in system | % | Ref. |
|---|---|---|---|
| (1) | (2) | (3) | |
| 47 | CGCG 436−030 (W) | 100 | 5 |
| 52 | NGC 6670 (W) | 62 | 1 |
| 53 | UGC 02369 (S) | 98 | 2 |
| 56 | NGC 5331 (S) | 81 | 1 |
| 57 | IRAS F06076−2139 (N) | 88 | 2 |
| 60 | IC 2810 (NW) | 68 | 1 |
| 63 | IRAS 18090+0130 (E) | 81 | 1 |
| 64 | III Zw 035 (N) | 100 | 5 |
| 67 | IRAS F16399−0937 (N) | 90 | 3 |
| 69 | IC 4687 (N,S)* | 66,22 | 1 |
| 75 | NGC 6090 (NE) | 90 | 4 |
| 79 | NGC 5256 (SW) | 63 | 2 |
| 80 | IRAS F03359+1523 (E) | 100 | 5 |
| 81 | ESO 550−IG025 (N) | 59 | 1 |
| 83 | MCG+12−02−001 (E,W)* | 90,10 | 2 |
| 95 | ESO 440−IG058 (S) | 89 | 1 |
| 104 | NGC 7771 | 90 | 1 |
| 105 | NGC 7592 (E,S)* | 63,0 | 2 |
| 106 | NGC 6286 | 87 | 1 |
| 107 | NGC 4922 (N) | 99 | 2 |
| 110 | NGC 3110 (NE) | 91 | 1 |
| 117 | MCG+08−18−013 (E) | 97 | 1 |
| 127 | MCG−03−34−064 | 75 | 1 |
| 141 | IC 0564 | 54 | 1 |
| 157 | MCG−02−33−098/9 (W) | 69 | 2 |
| 163 | NGC 4418 | 99 | 1 |
| 169 | ESO 343−IG013 (N) | 78 | 2 |
| 179 | NGC 7591 | 94 | 1 |
| 194 | ESO 432−IG006 (SW) | 63 | 1 |
| 196 | NGC 7753 | 64 | 1 |
Notes. Column (1): Name of the galaxy (galaxies) that emits most of the IR luminosity in a double (triple) system. Column (2): Percentage of IR emission originating in the dominant component. Column (3): Reference from which the contribution to the IR luminosity is derived. 1: Derived from Herschel data (as in Chu et al. 2017). 2: Derived from MIPS 24 data (as in Díaz-Santos et al. 2010). 3: MIR determination from Haan et al. (2011). 4: Predicted IR emission from radio continuum in Hattori et al. (2004). 5: We refer to the notes on individual objects in Appendix A.
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