Table 2.
Selected non-LBV supergiant variables in the LMC.
| HD | log Teff | log L/L⊙ (a) | Periods (d) | Ref. |
|---|---|---|---|---|
| 270920 | 3.748 | 5.50 | 250 | 1, 2 |
| 269018 | 4.057 | 5.02 | 14.6, 6.3, 32.5, 30.2 | 1, 2 |
| 33579 | 3.890 | 5.76 | 105, 81, 57, 70 | 1, 2 |
| 271182 | 3.775 | 5.57 | 260 | 1, 2 |
| 269541 | 3.877 | 5.24 | 8.1, 24.6, 12.0, 40.5 | 1, 2 |
| 269594 | 3.787 | 5.16 | 200 | 1, 2 |
| 269660 | 4.304 | 5.84 | 3.65, 10.8 | 1, 3 |
| 269697 | 3.797 | 5.31 | 48, 84 | 1, 2 |
| 269781 | 4.005 | 5.64 | 39.0 | 1, 3 |
| 268835 | 4.079 | 5.44 | 60, 380 | 4, 5 |
| 37974 | 4.352 | 5.90 | 24 | 4, 6 |
| 268757 | 3.739 | 5.42 | 540 | 7 |
| 268822 | 3.812 | 5.15 | 180 | 7 |
| 269612 | 3.86 | 4.93 | > 100 | 7 |
Notes.
Luminosities were derived from V magnitudes, assuming a mean extinction of 0.3 mag and a distance modulus of 18.50 mag and adopting bolometric corrections from Flower (1996).
References. (1) van Leeuwen et al. (1998); (2) McDonald et al. (2012); (3) Urbaneja et al. (2017); (4) van Genderen & Sterken (2002); (5) Stahl et al. (1983); (6) Zickgraf et al. (1985); (7) van Genderen et al. (2004).
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