Table 6.
Molecular gas mass.
| log10MH2 | fap | |
|---|---|---|
| Name | [M⊙] | |
| (1) | (2) | |
| VGS04 | < 7.83 | 1.05 |
| VGS11( * ) | 8.13 ± 0.16 | 1.43 |
| VGS19 | < 7.76 | 1.07 |
| VGS23 | 8.23 ± 0.10 | 1.40 |
| VGS26 | < 8.08 | 1.25 |
| VGS31 | 8.34 ± 0.10 | 1.20 |
| VGS31a | 9.12 ± 0.07 | 1.57 |
| VGS32 | 8.54 ± 0.07 | 1.57 |
| VGS34 | 8.90 ± 0.07 | 1.23 |
| VGS36 | < 8.14 | 1.19 |
| VGS39 | 8.26 ± 0.10 | 1.16 |
| VGS42 | 8.24 ± 0.13 | 1.17 |
| VGS44 | 8.21 ± 0.09 | 1.30 |
| VGS47 | 9.07 ± 0.07 | 1.46 |
| VGS49 | 8.66 ± 0.09 | 1.15 |
| VGS50( * ) | 8.22 ± 0.16 | 1.10 |
| VGS53 | 8.41 ± 0.09 | 1.28 |
| VGS56 | 8.36 ± 0.09 | 1.15 |
| VGS57 | 9.22 ± 0.07 | 1.45 |
| VGS58 | < 7.60 | 1.41 |
Notes. Column (1) is the molecular gas mass and total error. Column (2) is the aperture correction factor. ( * )The molecular gas mass of these galaxies has been derived from the CO(2−1) line emission intensity and the theoretical CO(2−1)-to-CO(1−0) line ratio estimated in Appendix A.
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