Table 1
Example object parameters.
| M⋆ (M⊙) | Age (kyr) | Luminosity (L⊙) | Tbol (K) | M10 000 AU (M⊙) | n0 (cm-3) | p | |
|
|
|||||||
| s4n109 | 5.1 | 1037 | 70.4 | 259 | 0.5 | 1.6 × 106 | 1.5 |
| s75n89 | 0.2 | 248 | 0.9 | 330 | 0.1 | 5.5 × 105 | 1.3 |
| s156n98 | 0.1 | 16 | 1.4 | 54 | 2.4 | 8.4 × 106 | 1.3 |
| s257n132 | 0.3 | 175 | 5.6 | 84 | 1.0 | 5.2 × 106 | 1.4 |
Notes. The first column is the protostellar mass, followed by its age and luminosity. Tbol is the bolometric temperature as defined by Myers & Ladd (1993). M10 000 AU is the gas mass within a radius of 10 000 AU from the protostar. Finally, n0 and p are the fitted parameters for the power law, ρ(r) = n0(r/ 100 AU)− p.
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