Table 4.
Results of the SED fitting with MBB and dusty torus models.
| Dust emission | ||
|---|---|---|
| log(Mdust/M⊙) | 8.64 ± 0.07 | |
| Mdust | (108 M⊙) | 4.4 ± 0.7 |
| Tdust | (K) | 71 ± 4 |
| β | 1.86 ± 0.12 | |
| LTIR, MBB | (1013 L⊙) | 2.48 |
| LTIR, MBB + Torus | (1013 L⊙) | 8.44 |
| GDR (a) | 101 ± 20 | |
Notes. SED fits are performed using two components, MBB and dusty torus (see Sect. 4.1). The table reports the individual contribution of the MBB component and the global contribution of MBB+torus for TIR (8–1000 μm).
Gas-to-dust mass ratio derived from Mdust (this work) and molecular mass M(H2) = (4.4 ± 0.2)×1010 M⊙ derived from CO(2-1) and (6-5) (Li et al. 2020; Feruglio et al. 2018).
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