Table 6
Ground-based CO data.
| Galaxy | CO J = 1−0 | Ref.a | CO J = 2−1 | Ref.a | CO J = 3−2 | Ref.a | |||||
| 115.271 GHz | 230.538 GHz | 345.796 GHz | |||||||||
|
|
|||||||||||
| NGC 34 | 5.6 ± 1.1 | 1,S | 10.1 ± 2.0 | 1, S | ··· | ··· | |||||
| IRASF 05189-2524 | 1.8 ± 0.5 | 3,A | 10.0 ± 2.6 | 3,I | 29.4 ± 7.2 | 3, J | |||||
| UGC 05101 | 1.8 ± 0.4 | 4,I | 9.7 ± 2.0 | 4, I | 22.5 ± 6.4 | 5, J | |||||
| NGC 5135 | 14.6 ± 3.5 | 3,I | 95 ± 21 | 3, I | 225 ± 56 | 3, J | |||||
| NGC 7130 | 12.4 ± 2.5 | 1,S | 44.8 ± 9.0 | 1, S | ··· | ··· | |||||
| NGC 7469 | 10.8 ± 2.6 | 2,I | 70.0 ± 16.4 | 2, I | 273.8 ± 65.2 | 2, J | |||||
Notes. Fluxes and 1σ uncertainties of ground-based observations of the low-J CO lines in units of 10-16 erg cm-2 s-1.
Reference for the CO line flux and telescope used. (A) ARO 12 m; (I) IRAM 30 m; (J) JCMT 15 m; (S) SEST 15 m.
Reference. (1) Albrecht et al. (2007). (2) Israel (2009). (3) Papadopoulos et al. (2012). (4) Pereira-Santaella et al. (2013). (5) Wilson et al. (2008).
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