Table 1.
YSOs observed with WWFI and effective temperatures, extinctions and distances from the literature.
Object (1) | α2000 | δ2000 | Teff | AV (2) | Distance (3) | Notes |
---|---|---|---|---|---|---|
[h:m:s] | [ ° :′:″] | [K] | [mag] | [pc] | ||
V397 Ori | 05:34:27.93 | −05:26:34.6 | 4205 | 0.28 | ![]() |
4 |
⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ |
V1313 Ori | 05:34:43.41 | −05:30:07.0 | 3849 | 0.97 | ![]() |
5 |
V1118 Ori | 05:34:44.74 | −05:33:42.1 | 3302 | 2.06 | 5, 6 | |
V1444 Ori | 05:34:45.19 | −05:25:04.1 | 4899 | 0.96 | ![]() |
5 |
... | ... | ... | ... | ... | ... | ... |
Notes. (1)Name of the YSO as listed in SIMBAD. (2)Extinctions from Manara et al. (2012). (3)Distance calculated by inverting the Gaia EDR3 parallax. (4)Effective temperatures calculated with the temperature scales of Kenyon & Hartmann (1995; K type stars) and Luhman et al. (2003; M type stars) with the spectral types from Hillenbrand et al. (2013). (5)Effective temperatures taken from Da Rio et al. (2012). (6)Distance set to the mean distance of the ONC (403 pc) determined by Kuhn et al. (2019). The full table is available at the CDS. A portion is shown here for guidance regarding its form and content.
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