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Table 4
Comparison between our adopted ISM extinction parameters (RV = 3.1) to thetotal to selective extinction ratio derived by Wegner (2003) for stars in common with our sample.
| Star | HD 24431 | HD 105627 | HD 153426 | HD 36861 A | HD 115455 | HD 135591 |
|---|---|---|---|---|---|---|
| (λ Orionis A) | ||||||
| E(B − V)(a) | 0.63 | 0.30 | 0.40 | 0.07 | 0.46 | 0.17 |
| E(B − V)(b) | 0.65 | 0.31 | 0.43 | 0.09 | 0.47 | 0.22 |
| RV (b) | 3.46 ± 0.06 | 3.24 ± 0.16 | 3.19 ± 0.16 | 2.46 ± 0.60 | 3.29 ± 0.13 | 3.57 ± 0.18 |
Notes. (a) Adopted in this work (see Table 1). (b)From Wegner (2003).
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