Open Access
Table 1
Program stars and properties of LOSs.
| Star | Name | Spectral type | E(B − V) (mag) | AV (mag) | Reference |
|---|---|---|---|---|---|
| BD+31°643 | ... | B5V | 0.86 ± 0.04 | 2.45 ± 0.15 | 1 |
| BD+40°4212 | Cyg OB2 3 | O9 | 1.90 | 5.89a | 2 |
| BD+40°4220 | Cyg OB2 5 | O7f | 1.99 | 6.17a | 3 |
| HD 23180 | o Per | B1III | 0.30 ± 0.04 | 0.93 ± 0.16 | 1 |
| HD 24432 | ... | B3II | 0.73 ± 0.04 | 2.02 ± 0.14 | 1 |
| HD 37022 | θ1 Ori C | O6V | 0.31 ± 0.05 | 1.78 ± 0.36 | 1 |
| HD 41690 | ... | B1V | 0.47 ± 0.04 | 1.37 ± 0.16 | 1 |
| HD 183143 | HT Sge | B7Iae | 1.27 | 3.94a | 3 |
Notes. (1) Valencic et al. (2004); (2) Leitherer et al. (1982); (3) Sonnentrucker et al. (2018) and Fan et al. (2019). (a)If adopting the total-to-selective extinction ratio of the Milky Way (RV = 3.1, Cardelli et al. 1989; Siebenmorgen et al. 2023).
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