Table 10
Estimates of effective temperatures (in kK) for different spectral types for the current sample (TAR), for supergiants in the LMC (Trundle et al. 2007, LMC), a sample of Galactic supergiants (Fraser et al. 2010, GAL) and for class Ia supergiants (Crowther et al. 2006, CLW).
| ST | TAR | LMC | GAL | CLW | ||||
|
|
||||||||
| O9.7 | 28.5 | – | – | 28.5 | ||||
| B0 | 27.0 | 28.5 | 28.0 | 27.5 | ||||
| B0.5 | 24.5 | 25.5 | 24.0 | 26.0 | ||||
| B0.7 | 23.5 | 23.5 | 23.0 | 22.5 | ||||
| B1 | 22.0 | 22.0 | 21.5 | 21.5 | ||||
| B1.5 | 20.5 | 20.5 | 19.5 | 20.5 | ||||
| B2 | 19.0 | 19.0 | 18.0 | 18.5 | ||||
| B2.5 | 17.5 | 17.5 | 17.0 | 16.5 | ||||
| B3 | 16.5 | 16.0 | 16.5 | 15.5 | ||||
| B5 | 13.5 | – | 15.0 | – | ||||
| B8 | 12.0 | – | 12.0 | – | ||||
Notes. The LMC sample has been rounded to the nearest 500 K to maintain consistency.
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