Open Access
Table 1
Models of pre-main sequence accreting stars from Baraffe et al. (2017; see text) used to produce the synthetic lcs.
| Models | M★ (M⊙) | R★ (R⊙) | T★ (K) | Ṁ (M⊙ yr−1) | Ṁcrit (M⊙ yr−1) | B★ (G) | RT (R★) |
|---|---|---|---|---|---|---|---|
| 1 | 0.165 | 0.950 | 3129 | 3.29 × 10−9 | 1.774 × 10−8 | 1571 | 9.71 |
| 2 | 0.178 | 0.944 | 3139 | 1.18 × 10−9 | 7.103×10−9 | 1021 | 10.02 |
| 3 | 0.202 | 1.033 | 3201 | 1.70 × 10−9 | 8.66×10−9 | 1040 | 9.55 |
| 4 | 0.236 | 0.953 | 3244 | 2.51 × 10−9 | 2.033 × 10−8 | 1832 | 10.91 |
| 5 | 0.237 | 1.127 | 3252 | 2.59 × 10−9 | 1.172 × 10−8 | 1129 | 9.24 |
| 6 | 0.288 | 1.318 | 3381 | 1.14 × 10−8 | 3.744 × 10−8 | 1742 | 8.43 |
| 7 | 0.348 | 1.370 | 3407 | 4.67 × 10−9 | 1.669 × 10−8 | 1162 | 8.63 |
| 8 | 0.459 | 1.530 | 3493 | 1.75 × 10−9 | 5.86×10−9 | 643 | 8.48 |
| 9 | 0.534 | 1.827 | 3579 | 4.83 × 10−9 | 1.039 × 10−8 | 712 | 7.47 |
| 10 | 0.556 | 1.791 | 3603 | 2.33 × 10−8 | 5.635 × 10−8 | 1717 | 7.72 |
| 11 | 0.614 | 1.873 | 3739 | 2.57 × 10−8 | 5.969 × 10−8 | 1713 | 7.63 |
| 12 | 0.708 | 1.940 | 3721 | 2.15 × 10−8 | 5.216 × 10−8 | 1588 | 7.73 |
| 13 | 0.715 | 1.783 | 3689 | 6.08 × 10−9 | 2.002 × 10−8 | 1096 | 8.43 |
| 14 | 0.832 | 1.689 | 4088 | 7.30 × 10−9 | 3.472 × 10−8 | 1604 | 9.37 |
| 15 | 0.923 | 2.251 | 4045 | 2.57 × 10−8 | 5.047 × 10−8 | 1386 | 7.27 |
| 16 | 1.072 | 2.255 | 4187 | 4.20 × 10−8 | 9.756 × 10−8 | 1996 | 7.63 |
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