Table 2
APEX CO(2-1) line fluxes and luminosities.
| Reg | Fint | S/N | Fint | L | L′ | MH2,CO |
| (Jy km s-1) | (10-17 W m-2) | (105L⊙) | (106 Kkms-1pc2) | (106M⊙) | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) |
|
|
||||||
| Host | 6.5 ± 1.3 | 5.1 | 0.0050 ± 0.0010 | 0.021 ± 0.004 | 5.4 ± 1.1 | 54.2 ± 10.7 |
Notes. (1) The entire host. (2) Integrated flux within dotted lines in Fig. 3. (3) Signal-to-noise ratio of the line. (4) Integrated flux in W m-2. (5) Line luminosity in solar luminosity. (6) Line luminosity using Eq. (3) in Solomon et al. (1997). (7) Molecular gas mass estimated assuming 
(see Sect. 3) and the Galactic CO-to-H2 conversion factor αCO = 5 M⊙/ (K km s-1 pc2).
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