Table 8
OH maser luminosities and CO luminosities for some of the sources in the sample.
| Galaxy | log LOH | L CO1−0 |
|
| [L⊙] | [108 K km s-1 pc2] |
|
|
|
|
|||
| Arp 220 | 2.58 | 78.5 | 4.8 |
| IC 342 | None | ... | ... |
| IC 694/NGC 3690 | 1.38 | 29 | 0.83 |
| IC 860 | 0.27a | 3.07b | 0.61 |
| I17208 | 3.04 | 146.9 | 7.5 |
| M82 | –1.7 | 5.7 | 0.0035 |
| NGC 253 | –1.3 | 4.6 | 0.011 |
| NGC 1068 | –0.3 | 20.7 | 0.024 |
| NGC 1365 | None | ... | ... |
| NGC 1614 | None | ... | ... |
| NGC 2146 | None | ... | ... |
| NGC 3079 | Abs. | ... | ... |
| NGC 4418 | 0.04a | 1.03c | 1.1 |
| NGC 4945 | Abs. | ... | ... |
| NGC 5135 | None | ... | ... |
| NGC 7130 | None | ... | ... |
| UGC 5101 | 1.61 | 50.8 | 0.80 |
Notes. Data are from Darling (2007) unless stated otherwise below. The note "None" in the LOH column indicates that Darling (2007) has not detected any OH megamaser emission, and “Abs.” that an OH absorber is detected. The names of the HC3N-luminous galaxies are written in boldface. The HC3N/HCN values for IC 342 and M82 are probably overestimated (see Appendix A.1).
From Albrecht et al. (2007).
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