Table 1
Overview of the simulated protostars studied in this work.
| Sink | Mfinal (M⊙) | Menv (M⊙) | tff (kyr) | I/C |
|---|---|---|---|---|
| M022–C | 0.22 | 1.50 | 144.5 | C |
| M023–I | 0.23 | 0.90 | 186.4 | I |
| M048–C | 0.48 | 1.06 | 171.6 | C |
| M048–I | 0.48 | 1.19 | 162.2 | I |
| M049–C | 0.49 | 0.73 | 206.5 | C |
| M072–I | 0.72 | 0.85 | 192.2 | I |
| M072–C | 0.72 | 5.58 | 74.8 | C |
| M073–C | 0.73 | 0.94 | 182.5 | C |
| M101–C | 1.01 | 1.74 | 134.1 | C |
Notes.Isolated and clustered sources are denoted I and C, respectively. The envelope mass, Menv, is the total mass within a 10 000 au sphere at the onset of collapse (i.e., at the moment the sink particle is formed). The free-fall timescale is calculated assuming a uniform density within 10 000 au. The quantity Mfinal indicates the final mass at the end of the simulation.
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