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Table 3
SED fitting parameters.
| Component | SpT | Teff1 | AV (mag) | L 2 | Mass | IR ex.33 | |
| (K) | fit | (L⊙) | (M⊙) | (mag) | |||
|
|
|||||||
| LkCa 3 A | M2 | 3490 |
|
0.75 | 0.511 | 1.6 | |
| LkCa 3 B | K7 | 3970 |
|
0.49 | 1.200 | 1.0 | |
| DD Tau A | M3 | 3360 |
|
0.15 | 0.274 | 6.8 | |
| DD Tau B | M3 | 3360 |
|
0.27 | 0.993 | 3.8 | |
| LkCa 7 A | M0 | 3770 |
|
0.39 | 0.536 | – | |
| LkCa 7 B | M3.5 | 3260 |
|
0.23 | 0.259 | – | |
| FV Tau A | K5 | 4140 |
|
0.29 | 1.294 | 5.4 | |
| FV Tau B | K6 | 4020 |
|
0.16 | 1.041 | 4.9 | |
| FV Tau/c A | M2.5 | 3425 |
|
0.16 | 0.343 | – | |
| FV Tau/c B | M3.5 | 3260 |
|
0.03 | 0.234 | – | |
| UX Tau A | K5 | 4140 |
|
0.86 | 1.005 | 3.9 | |
| UX Tau B | M2 | 3490 |
|
0.27 | 1.032 | 0.1 | |
| UX Tau C | M5 | 2880 |
|
0.01 | 0.087 | 1.5 | |
| FX Tau A | M1 | 3630 |
|
0.34 | 0.514 | 4.7 | |
| FX Tau B | M4 | 3160 |
|
0.19 | 0.180 | 3.4 | |
| DK Tau A | K9 | 3880 |
|
0.36 | 0.552 | 7.2 | |
| DK Tau B | M1 | 3630 |
|
0.55 | 1.315 | 3.7 | |
| XZ Tau A | M2 | 3490 |
|
0.15 | 0.334 | – | |
| XZ Tau B | M3.5 | 3260 |
|
0.07 | 0.228 | – | |
| HK Tau A | M1 | 3630 |
|
0.13 | 0.423 | – | |
| HK Tau B | M2 | 3490 |
|
0.03 | 0.334 | – | |
| V710 Tau A | M0.5 | 3700 |
|
0.37 | 0.567 | – | |
| V710 Tau B | M2.5 | 3425 |
|
0.27 | 1.258 | – | |
| UZ Tau A | M2 | 3490 |
|
0.50 | 0.417 | 5.4 | |
| UZ Tau B | M3 | 3360 |
|
0.35 | 0.482 | 4.5 | |
| UZ Tau C | M1 | 3630 |
|
0.30 | 0.715 | 3.1 | |
| GH Tau A | M2 | 3490 |
|
0.29 | 0.360 | 4.5 | |
| GH Tau B | M2 | 3490 |
|
0.37 | 0.511 | 3.0 | |
| HN Tau A | K5 | 4140 |
|
0.15 | 0.715 | – | |
| HN Tau B | M4 | 3160 |
|
0.02 | 0.190 | – | |
| HV Tau A | M2 | 3490 |
|
0.31 | 0.458 | 1.6 | |
| HV Tau C | M0 | 3770 |
|
0.08 | 0.572 | 2.6 | |
| V999 Tau A | M0.5 | 3700 |
|
0.27 | 0.567 | – | |
| V999 Tau B | M2.5 | 3425 |
|
0.21 | 0.897 | – | |
| V1000 Tau A | M1 | 3630 |
|
0.24 | 0.564 | – | |
| V1000 Tau B | K7 | 3970 |
|
0.15 | 0.722 | – | |
| RW Aur A | K2 | 4760 |
|
0.21 | 1.155 | 6.3 | |
| RW Aur B | K5 | 4140 |
|
0.81 | 1.294 | 1.6 | |
Notes.
(1)
The effective temperature was calculated from the spectral type, and the masses were obtained using the 2 Myr isochrones from Baraffe et al. (2015).
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