Table 3
Spitzer data.
| Galaxy | f5.8/f3.6a | H2/7.7 μmb | f 24 μm,tot c | f 24 μm,CObeam d |
| [mJy] | [mJy] | |||
|
|
||||
| HCG 6b | –0.25 | 0.198 | 3.80 ± 0.19 | 2.53 ± 0.08 |
| HCG 6c | –0.38 | – | 0.80 ± 0.04 | 1.32 ± 0.08 |
| HCG 15a | –0.29 | 0.044 | 5.60 ± 0.28 | 4.20 ± 0.09 |
| HCG 15d | –0.30 | 0.112 | 2.70 ± 0.14 | 3.72 ± 0.10 |
| HCG 25b | –0.24 | 0.098 | 4.70 ± 0.24 | 5.69 ± 0.07 |
| HCG 25f | –0.36 | – | – | 0.70 ± 0.07 |
| HCG31ac | 0.32 | 0.002 | – | 307.68 ± 0.14 |
| HCG 40b | –0.34 | 0.083 | 3.00 ± 0.15 | 9.07 ± 0.07 |
| HCG 40c | 0.09 | 0.010 | 73.40 ± 3.67 | 35.08 ± 0.07 |
| HCG 40d | 0.06 | 0.013 | 88.10 ± 4.41 | 67.71 ± 0.07 |
| HCG 44a | –0.20 | 0.042(1) | 246.00 ± 12.30 | 73.85 ± 0.06 |
| HCG 44d | 0.19 | 0.021 | 79.90 ± 4.00 | 19.80 ± 0.06 |
| HCG 47a | –0.01 | 0.035 | 87.00 ± 4.35 | 38.00 ± 0.13 |
| HCG 47d | –0.19 | – | 4.50 ± 0.23 | 4.70 ± 0.13 |
| HCG 55c | –0.01 | 0.018 | 7.70 ± 0.39 | 6.13 ± 0.07 |
| HCG 56b | 0.16 | 0.053 | 185.00 ± 9.25 | 134.56 ± 0.07 |
| HCG 56c | –0.32 | 0.037 | 0.90 ± 0.05 | 10.39 ± 0.07 |
| HCG 57a | –0.27 | 0.174 | 13.80 ± 0.69 | 9.63 ± 0.05 |
| HCG 57d | 0.03 | – | 24.00 ± 1.20 | 15.50 ± 0.05 |
| HCG 67b | 0.02 | 0.006 | 84.80 ± 4.24 | 32.65 ± 0.07 |
| HCG 68a | –0.35 | 0.741 | 21.30 ± 1.07 | 14.63 ± 0.05 |
| HCG 68b | –0.35 | 0.073 | 9.80 ± 0.49 | 7.79 ± 0.05 |
| HCG 68c | 0.01 | 0.044 | 403.60 ± 20.18 | 122.81 ± 0.06 |
| HCG 79a | –0.06 | 0.011 | 23.30 ± 1.17 | 17.25 ± 0.05 |
| HCG 79b | –0.18 | 0.010 | 33.70 ± 1.69 | 27.95 ± 0.05 |
| HCG 82b | –0.31 | 0.045 | 5.80 ± 0.29 | 3.76 ± 0.04 |
| HCG 82c | 0.41 | 0.014 | 90.60 ± 4.53 | 63.30 ± 0.04 |
| HCG 91a | 0.09 | 0.030 | 351.00 ± 17.55 | 184.46 ± 0.06 |
| HCG 95a | –0.08 | 0.071 | 19.80 ± 0.99 | 15.17 ± 0.07 |
| HCG 96c | 0.37 | 0.007 | – | 473.06 ± 1.40 |
| HCG100a | –0.05 | 0.013 | 153.00 ± 7.65 | 102.47 ± 0.08 |
Notes.
Value taken from Roussel et al. (2007).
Ratio between luminosity of the total (sum of S(0)–S(3) lines) warm H2 emission and the 7.7 μm PAH feature. If H2/7.7 μm > 0.04 the galaxy is classified as a MOHEG (Ogle et al. 2010).
Total 24 μm flux of the galaxy and its error, taken from Bitsakis et al. (2011).
24 μm flux within the IRAM CO(1–0) beam (see text) and its photometric error, derived from the rms of the background. In addition, a calibration error of 10% error (Engelbracht et al. 2007) has to be taken into account.
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