Table 6
Stellar masses obtained from the velocity profile fits and values from the literature.
| Source | This work | Literature | ||
|---|---|---|---|---|
| M⋆ (M⊙) (a) | Molecule | M⋆ (M⊙) | Method | |
| [GY92] 197 | 0.23 ± 0.02 | C17O | ||
| Elias 29 | 2.5 ± 0.6 (b) | HCO+ J = 3−2 emission | ||
| IRS 43 | 4.0 ± 0.3 | C34S | 1.80 ± 0.42 (c) | HCN J = 3−2 emission |
| 3.9 ± 0.7 | C17O | |||
| IRS 44 | 1.2 ± 0.1 | H13CO+ | ||
| IRAS 16253-2429 | 0.03 ± 0.02 | C17O (infalling) | 0.03 ± 0.01 (d) | C18O J = 2−1 emission |
| IRS 67 (e) | 2.2 ± 0.2 | C17O | ||
Notes. (a) The stellar masses were calculated assuming aninclination of 70°. (b) From Lommen et al. (2008). (c) From Brinch et al. (2016), for the binary system. (d)From Yen et al. (2017). (e)A more detailed analysis of IRS 67 is presented in Artur de la Villarmois et al. (2018).
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