Table 2
CO line parameters and intensities.
| Galaxy | Line | Center | θ FWHM | T mb | V | ΔV | I CO | L CO | Reference |
| (′′) | (mK) | (km s-1) | (km s-1) | (K km s-1) | (L⊙) | ||||
|
|
|||||||||
| Haro 11 | CO(1–0) | 30 (1) | <10.7 (a) | – | – | <0.69 | <6.6 × 103 | this work | |
| CO(2–1) | 26 (2) | 8.63 | 6113 | 59 | 0.54 ± 0.19 | 3.2 × 104 | this work | ||
| CO(3–2) | 17 (2) | 7.20 | 6103 | 63 | 0.48 ± 0.17 | 4.0 × 104 | this work | ||
| Mrk 1089 | CO(1–0) | 21 (3) | 26.3 | 3987 | 148 | 2.56 ± 0.50 | 4.7 × 103 | Leon et al. (1998) | |
| CO(2–1) | 26 | 14.1 | 3990 | 111 | 1.67 ± 0.40 | 3.8 × 104 | this work | ||
| CO(3–2) | 17 | 11.5 | 3976 | 95 | 1.16 ± 0.32 | 3.8 × 104 | this work | ||
| Mrk 930 | CO(1–0) | 21 | 2.17 | 5491 | 62 | 0.14 ± 0.07 | 4.7 × 102 | this work | |
| CO(2–1) | 11 (3) | <6.44 | – | – | <0.34 | <2.6 × 103 | this work | ||
| NGC 4861 | CO(1–0) | 21 | <6.51 | – | – | <0.35 | <1.1 × 101 | this work | |
| CO(1–0) | total(b) | – | – | – | <1.23 | <3.9 × 101 | this work | ||
| CO(2–1) | 11 | <8.74 | – | – | <0.47 | <3.3 × 101 | this work | ||
| NGC 625 | CO(1–0) | (0, + 30′′) | 30 | <24.9 | – | – | <1.86 | <3.3 × 101 | this work |
| CO(1–0) | (0, + 15′′) | 30 | 29.0 | 373 | 72 | 2.23 ± 0.72 | 4.0 × 101 | this work | |
| CO(1–0) | (0,0) | 30 | 27.1 | 379 | 71 | 2.05 ± 0.63 | 3.6 × 101 | this work | |
| CO(1–0) | (0, − 15′′) | 30 | <21.6 | – | – | <1.61 | <2.9 × 101 | this work | |
| CO(1–0) | total(b) | 57.7 | 374 | 70 | 4.26 ± 0.62 | 7.5 × 101 | this work | ||
| CO(1–0) | ref(c) | 30 | – | – | – | <1.61(c) | <2.9 × 101 | this work | |
| CO(2–1) | 22 (4) | 58.0 | 390 | 27 | 1.64 ± 0.40 | 1.0 × 102 | Cannon (2004) | ||
| CO(3–2) | 17 | 59.0 | 381 | 23 | 1.44 ± 0.38 | 2.2 × 102 | this work | ||
| UM 311 | CO(1–0) | 30 | <11.4 | – | – | <0.61 | <4.1 × 102 | this work | |
| CO(1–0) | total(b) | – | – | – | <3.05 | <2.0 × 103 | this work | ||
| CO(2–1) | 26 | 10.9 | 1678 | 41 | 0.47 ± 0.15 | 1.9 × 103 | this work | ||
| CO(3–2) | 17 | 8.62 | 1686 | 44 | 0.40 ± 0.14 | 2.3 × 103 | this work | ||
Notes. (1) ATNF/Mopra; (2) APEX/SHeFI; (3) IRAM/30-m; (4) JCMT/RxA.(a)The upper limits are 3σ. (b) Total emission for extended galaxies, estimated from the other Mopra pointings for NGC 625 and extrapolated from the 100μm continuum emission for NGC 4861 and UM 311 (see Sect. 3.2). (c) Estimated CO(1–0) line intensity at the position covered by the CO(2–1) and CO(3–2) lines.
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