Table 4.
Measured parameters of the observed stars with the spectral types adopted in this work and the most precise spectral types available in the literature.
| Stars | Teff (K) | log (g) | SpT (tw) | SpT |
|---|---|---|---|---|
| HD 240015 | 24 000 ± 2000 | 3.0 ± 0.2 | B0.5II | Be |
| HD 240016 | 21 000 ± 1000 | 3.0 ± 0.2 | B1.5II | B |
Notes. The spectral types of the stars determined in this work (tw) are given in the fourth column. We adopted the spectral types following Hohle et al. (2010), and the literature spectral types are from Chick et al. (2020).
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