Table 4
Physical parameters for a subset of YSO candidates with at least five photometric data points.
ID | Model set(a) | Class | R* (R⊙) | T* (K) | L* (L⊙) | M*(b) (M⊙) | Age(b) (Myr) | Note(c) |
---|---|---|---|---|---|---|---|---|
1 | sp–s-i | II/III | 5.2 | 3592 | 4.0 | … | … | |
2 | sp–s-i | II/III | 2.6 | 6791 | 13.2 | … | … | TP01 |
4 | s–s-i | star | 1.2 | 2955 | 0.1 | … | … | |
5 | s–s-i | star | 1.0 | 3388 | 0.1 | … | … | |
6 | s–s-i | star | 1.0 | 5120 | 0.6 | … | … | TP03 |
9 | sp–h-i | II/III | 3.3 | 3359 | 1.2 | … | … | |
10 | s-pbhmi | 0 | 25.8 | 6214 | 892.1 | 8.0 | 0.06 | TP06 |
11 | s–s-i | star | 1.2 | 2955 | 0.1 | … | … | |
12 | spubsmi | I | 23.0 | 6194 | 702.1 | … | … | TP07 |
13 | sp–h-i | II/III | 2.6 | 6112 | 8.4 | … | … | TP09 |
14 | sp–h-i | II/III | 3.6 | 3736 | 2.2 | … | … | |
15 | sp–h-i | II/III | 10.3 | 7101 | 244.9 | … | … | TP08 |
Notes.(a) See Table 3 footnotes for the description of the model set names.(b) We provide stellar masses (M*) and ages only for sources with reliable estimation of these parameters (see text for details).(c) IDs of the YSO candidates in Gy 3–7 identified by Tapia et al. (1997), see Fig. 1.
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