Table 5
Calculated disc masses for Tdust = 15 K and values from the literature.
| Source | Mdisc (10−3 M⊙) | |
|---|---|---|
| This work | Literature | |
| GSS30-IRS1 | 6.2 ± 0.6 | |
| [GY92] 30 | 18.5 ± 1.6 | |
| WL 12 | 28.3 ± 2.4 | 11 (a) |
| LFAM 23 | 3.1 ± 0.3 | |
| [GY92] 197 | 22.6 ± 2.0 | |
| Elias 29 | 7.3 ± 0.6 | 11 (a) |
| <7 (b) | ||
| IRS 43 VLA 1 | 7.3 ± 0.7 | 8 (a) |
| IRS 43 VLA 2 | 1.3 ± 0.2 | |
| IRS 44 | 6.8 ± 0.6 | |
| IRAS 16253-2429 | 7.0 ± 0.6 | |
| ISO-Oph 203 | 2.0 ± 0.2 | |
| IRS 67 A | 6.3 ± 1.3 | |
| IRS 67 B | 27.4 ± 2.5 | |
Notes. The errors in the second column do not include uncertainties in the assumed dust temperature (Tdust = 15 K), but the disc masses decrease by a factor of ~3 when a dust temperature of 30 K is assumed. (a)From Jørgensen et al. (2009) at 1.1 mm, with Tdust = 30 K. (b) From Lommen et al. (2008) at 1.1 mm, with Tdust = 30 K.
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