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Table 3

Adopted parameters and bolometric luminosities for the cool supergiants.

Hosek Damineli
ID SpT Teff
(K)
AKs
(mag)
log(L/L)
(dex)
AKs
(mag)
log(L/L)
(dex)
W237 M3-4I 3550 0.54 5.20 0.66 5.24
W20 M3-4I 3550 0.76 4.98 0.93 5.04
W75 M1 Ia 4000 1.01 5.14 1.24 5.22
W26 M1-1.5 Ia 3780 0.54 5.35 0.66 5.39
W4 F3 Ia+ 6700 0.49 5.25 0.61 5.29
W8a F8 Ia+ 6200 1.26 5.47 1.55 5.56
W32 F5 Ia+ 6500 0.61 5.45 0.74 5.49
W16a A5 Ia+ 8200 0.63 5.40 0.77 5.45
W12a F1 Ia+ 7150 0.66 5.22 0.81 5.27
W265 F1-5 Ia+ 6750 0.69 5.18 0.69 5.23

Notes. Extinction and luminosities are derived using the extinction laws of Hosek et al. (2018) and Damineli et al. (2016). For reference, Beasor et al. (2021) adopted a cluster average extinction of AK = 0.74 ± 0.08 for Wd1.

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