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Table 2
Overview of the simulation names, stellar masses and effective temperatures, number of initial embryos Nemb,ini, and number of simulation runs for all simulations discussed in this work.
| Name | M⋆ |  |
Nemb,ini | Simulations |
|---|---|---|---|---|
| NGM10 | 0.1 M⊙ | 2811 K | 50 | 1000 |
| NGM14 | 0.3 M⊙ | 3416 K | 50 | 997 |
| NGM11 | 0.5 M⊙ | 3682 K | 50 | 1000 |
| NGM12 | 0.7 M⊙ | 4430 K | 50 | 999 |
| NG75(b) | 1.0 M⊙ | 5731 K | 50 | 1000 |
| NG76(b) | 1.0 M⊙ | 5731 K | 100 | 1000 |
| NGM17(c) | 0.1 M⊙ | 2811 K | 1 | 10000 |
| NGM21(c) | 0.1 M⊙ | 2811 K | 1 | 9867 |
| NGM22(c) | 0.1 M⊙ | 2811 K | 1 | 9939 |
Notes. (a) Following Baraffe et al. (2015). (b)Also discussed in Paper II. (c)With modified parameters (see Sect. 4.1.2).
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