Table 2
A comparison with stellar parameters from the literature and luminosities as derived with the assumption that RV = 5.
Literature | RV = 5 | RV = 3.1 | ||||
Name | AV | log L∗ | Mass | Ref. | log L∗ | log L∗ |
[L⊙] | [M⊙] | [L⊙] | [L⊙] | |||
|
||||||
PDS 204 | 3.0 | 3.06 | – | H08 | 4.76 | 3.67 |
MWC 789 | 0.7 | 2.31 | 3.9 | H04 | 2.23 | 2.14 |
LkHα 208 | 1.2 | 1.78 | 2.4 | H04 | 1.79 | 1.61 |
LkHα 339 | 4.3 | 2.08 | 3.4 | H04 | 1.80 | 1.36 |
MWC 137 | 4.5 | 4.46 | 18.9 | H92 | 5.35 | 4.42 |
LkHα 215 | 3.2 | 3.24 | 6.6 | H04 | 3.16 | 2.79 |
MWC 147 | 2.0 | 3.50 | 9.7 | H04 | 3.41 | 3.26 |
R Mon | 4.3 | 3.55 | 10.4 | H92 | 2.71 | 2.12 |
Hen 3-331 | 1.0 | 3.7 | 9 | Mi01 | 4.40 | 4.17 |
V921 Sco | 4.8 | 4.0 | 9 | B07 | 5.90 | 4.83 |
MWC 878 | – | 5.3 | 30 | Mi01 | 5.30 | 4.77 |
LkHα 260 | 2.3 | 2.57 | – | DW97 | 3.30 | 2.65 |
MWC 297 | 7.7 | 4.05 | 10 | D97 | 5.71 | 3.92 |
AS 310 | 6.6 | 5.43 | 43.5 | H04 | 5.00 | 4.23 |
Notes. The last column repeats our derived values with RV = 3.1 to accommodate the comparison. The table gives an assessment of typical conservative uncertainties on the stellar parameters. The reference abbreviations are identical to those defined in the footnote of Table 1.
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