Table 7
H2 masses using CO observations, dust measurements, and models.
| Galaxy | From CO observations | From dust | From LTE | From Cloudy | |||||
|
|
|||||||||
| X CO / X CO,gal (a) | MH2 (M⊙) | MH2 (M⊙) | (M⊙) |
MH2 (M⊙) | |||||
|
|
|
||||||||
| CO(1–0) | R21 = 0.8(b) | R31 = 0.6(c) | Average | CO-free | CO-traced | ||||
|
|
|||||||||
| Haro 11 | 1 | <4.4 × 108 | 3.3 × 108 | 1.7 × 108 | 2.5 × 108 | 3.6 × 109 | >3.6 × 106< 2.4 × 108 | 1.2 × 108 | 1.6 × 109 |
| 10 | <4.4 × 109 | 3.3 × 109 | 1.7 × 109 | 2.5 × 109 | – | ||||
| Mrk 1089 | 1 | 3.1 × 108 | 3.9 × 108 | 1.6 × 108 | 2.9 × 108 | 8.3 × 108 | |||
| 16 | 4.9 × 109 | 6.2 × 109 | 2.5 × 109 | 4.5 × 109 | – | ||||
| Mrk 930 | 1 | 3.1 × 107 | <9.8 × 107 | – | 3.1 × 107 | 1.0 × 109 | |||
| 22 | 6.8 × 108 | <2.1 × 109 | – | 6.8 × 108 | – | ||||
| NGC 4861 | 1 | <7.3 × 105 | <1.2 × 106 | – | <7.3 × 105 | – | |||
| 42 | <3.1 × 107 | <5.1 × 107 | – | <3.1 × 107 | – | ||||
| Total | 1 | <2.6 × 106 | – | – | <2.6 × 106 | 1.7 × 108 | |||
| NGC 625 | 1 | <1.9 × 106 | 1.1 × 106 | 9.0 × 105 | 1.0 × 106 | – | |||
| 9 | <1.7 × 107 | 9.7 × 106 | 8.2 × 106 | 9.0 × 106 | – | ||||
| Total | 1 | 5.0 × 106 | – | – | 5.0 × 106 | 9.4 × 107 | >5.8 × 103< 5.7 × 105 | ||
| UM 311 | 1 | <2.7 × 107 | 2.0 × 107 | 9.4 × 106 | 1.5 × 107 | – | |||
| 4 | <1.2 × 108 | 8.5 × 107 | 4.1 × 107 | 6.3 × 107 | – | ||||
| Total | 1 | <1.3 × 108 | 9.8 × 107 | – | 9.8 × 107 | 3.3 × 109 | |||
Notes. The H2 masses from CO observations are measured within the CO beams. For extended galaxies, we also consider the estimated total CO emission (see Sect. 3.2 for details). (a) Ratio of our adopted XCO value to the Galactic value XCO,gal. To bracket the range of molecular gas masses, there are two lines for each galaxy corresponding to the molecular masses derived with two values of the XCO factor: XCO = XCO,gal (lower mass case) and XCO = XCO,Z ∝ Z-2 (upper mass case). (b)R21 is the CO(2–1)/CO(1–0) ratio. (c)R31 is the CO(3–2)/CO(1–0) ratio.
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