Table 5.
Stellar and accretion parameters of the Class I sample.
| ID | Age | rK | Lbol | AV | Macc. | L⋆ | Teff | SpT | M⋆ | R⋆ | Ṁacc |
|---|---|---|---|---|---|---|---|---|---|---|---|
| [L⊙] | [mag] | [L⊙] | [L⊙] | [K] | [M⊙] | [R⊙] | [10−8 M⊙ yr−1] | ||||
| 149 | BL | 3–8 | 0.31 | 44.5–51.0 | 0.05–0.10 | 0.25–0.30 | 2818–2754 | M7.5 | 0.13–0.11 | 2.2–2.1 | 3.2–8.3 |
| 1 Myr | 43.0–49.5 | 0.04–0.08 | 0.26–0.31 | 3075–3038 | M5.5 | 0.20–0.17 | 1.8–1.6 | 1.4–3.2 | |||
| 181 | BL | 3–8 | 1.11 | 31.5–34.5 | 0.60–0.86 | 0.25–0.51 | 3020–2754 | M6-M7.5 | 0.19–0.11 | 2.5–2.1 | 32–70 |
| 1 Myr | 31.0–34.0 | 0.57–0.81 | 0.30–0.54 | 3218–3075 | M4.5-M5.5 | 0.25–0.20 | 2.1–1.8 | 19–31 | |||
| 186 | BL | 3–8 | 18.2 | 45.0–51.0 | 2.46–5.08 | 13.1–15.7 | 5248–5248 | G9.5 | 2.84 | 4.5 | 16–33 |
| 1 Myr | 45.5–52.0 | 2.62–5.7 | 12.5–15.6 | 5019–4942 | K1-K1.5 | 3.03–2.80 | 4.9–4.5 | 18–38 | |||
| 191 | BL | 3–8 | 58.8 | 33.0–38.0 | 16.4–29.9 | 28.9–42.5 | 5754–5623 | G5.5-G7 | 3.07–2.95 | 5.7–5.3 | 120–220 |
| 1 Myr | 34.0–39.0 | 18.5–33.7 | 25.1–40.4 | 5395–5173 | G9.5-K0 | 3.53–3.28 | 2.1–1.8 | 19–31 | |||
| 200 | BL | 3–8 | 7.63 | 36.0–41.0 | 2.19–4.01 | 3.62–5.44 | 3981–3802 | K8-M0.5 | 0.70–0.53 | 4.7–3.9 | 60–120 |
| 1 Myr | 34.0–39.5 | 1.72–3.34 | 4.29–5.91 | 4683–4547 | K3.5-K4.5 | 1.90–1.52 | 3.5–3.1 | 13–28 | |||
| 202 | BL | 1–3 | 0.23 | 17.0–22.5 | 0.02–0.04 | 0.19–0.21 | 2754–2754 | M7.5 | 0.11 | 2.1 | 1.7–3.3 |
| 1 Myr | 15.5–21.5 | 0.02–0.04 | 0.20–0.22 | 3002–3002 | M6 | 0.15 | 1.4 | 0.7–1.4 | |||
| 204 | BL | 3–8 | 0.51 | 38.0–41.0 | 0.24–0.34 | 0.17–0.27 | 2754–2754 | M7.5 | 0.11 | 2.1 | 19–28 |
| 1 Myr | 36.5–40.5 | 0.20–0.32 | 0.19–0.31 | 3075–3002 | M5.5-M6 | 0.20–0.15 | 1.8–1.4 | 7–13 | |||
| 215 | BL | 1–3 | 0.12 | 20.0–25.5 | 0.02–0.03 | 0.09–0.11 | 2754–2754 | M7.5 | 0.11 | 2.1 | 1.4–2.6 |
| 1 Myr | 19.0–24.0 | 0.01–0.03 | 0.09–0.11 | 2928–2928 | M6.5 | 0.10 | 1.0 | 0.6–1.2 | |||
| 231 | BL | 1–3 | 0.59 | 27.5–34.0 | 0.03–0.07 | 0.52–0.56 | 3020–3020 | M6 | 0.19 | 2.5 | 1.6–3.6 |
| 1 Myr | 26.0–32.5 | 0.03–0.06 | 0.53–0.56 | 3289–3218 | M4-M4.5 | 0.28–0.25 | 2.2–2.1 | 0.8–1.9 | |||
| 232 | BL | 1–3 | 0.70 | 14.0–20.0 | 0.07–0.15 | 0.55–0.63 | 3090–3020 | M5.5-M6 | 0.22–0.19 | 2.5 | 3.6–8.1 |
| 1 Myr | 12.5–18.5 | 0.06–0.13 | 0.57–0.64 | 3289–3289 | M4 | 0.28 | 2.2 | 2.0–4.2 |
Notes. The first two parameters of the table (the age and the K-band veiling, rK) are assumed. The bolometric luminosity is derived in Appendix F, while for all the other parameters the range of values derived from our method, as described in Sect. 5.1 is reported. BL denotes the birthline of Palla & Stahler (1993).
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