| 1SpT . | 5L* . | 5M* . | 5age . | 2Teff . | 3d . | 4σd . | 6AV . |
|---|---|---|---|---|---|---|---|
| . | (L⊙) . | (M⊙) . | Myr . | (K) . | (pc) . | (pc) . | (mag) . |
| F2 | 10 | 1.67 | 10 | 6900 | 162 | 2 | 1.9 |
| 1SpT . | 5L* . | 5M* . | 5age . | 2Teff . | 3d . | 4σd . | 6AV . |
|---|---|---|---|---|---|---|---|
| . | (L⊙) . | (M⊙) . | Myr . | (K) . | (pc) . | (pc) . | (mag) . |
| F2 | 10 | 1.67 | 10 | 6900 | 162 | 2 | 1.9 |
References: 1. Herbig 1960; Natta et al. 2001 2. Testi et al. 2001 3. Gaia Collaboration 2016 4. Bailer-Jones et al. 2018 5. The luminosity L = 6.6 L⊙ from Garcia Lopez et al. 2006 (d = 130 pc) is re-scaled considering the new distance from GAIA; the value of mass and age considering the new luminosity where derived using the tracks of Siess, Dufour & Forestini (2000). 6. The extinction was measured by fitting the SED shown in Fig. 4.
| 1SpT . | 5L* . | 5M* . | 5age . | 2Teff . | 3d . | 4σd . | 6AV . |
|---|---|---|---|---|---|---|---|
| . | (L⊙) . | (M⊙) . | Myr . | (K) . | (pc) . | (pc) . | (mag) . |
| F2 | 10 | 1.67 | 10 | 6900 | 162 | 2 | 1.9 |
| 1SpT . | 5L* . | 5M* . | 5age . | 2Teff . | 3d . | 4σd . | 6AV . |
|---|---|---|---|---|---|---|---|
| . | (L⊙) . | (M⊙) . | Myr . | (K) . | (pc) . | (pc) . | (mag) . |
| F2 | 10 | 1.67 | 10 | 6900 | 162 | 2 | 1.9 |
References: 1. Herbig 1960; Natta et al. 2001 2. Testi et al. 2001 3. Gaia Collaboration 2016 4. Bailer-Jones et al. 2018 5. The luminosity L = 6.6 L⊙ from Garcia Lopez et al. 2006 (d = 130 pc) is re-scaled considering the new distance from GAIA; the value of mass and age considering the new luminosity where derived using the tracks of Siess, Dufour & Forestini (2000). 6. The extinction was measured by fitting the SED shown in Fig. 4.
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