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Table 1

Single-cloud lines-of-sight properties.

Star ISM
Identifier Spectral type v sin(i) E(B–V)a RV Ref f(H2)c Na I-UV velocity 5797/5780d
(km s−1) (mag) (km s−1)
HD 23180 B1 III 100 0.28 3.11 V04 0.51 13.8 ± 0.3 0.73 (ζ)
HD 24398 B1 Ib 43 0.29 2.63 W03 0.60 14.2 ± 0.2 0.53 (ζ)
HD 203532 B3 IV 0.30 3.37 V04 0.84 15.2 ± 0.2 0.48 (ζ)
HD 149757 O9.2 IVnn 303 0.32 2.55 V04 0.63 –14.2 ± 0.5 0.43 (ζ)
HD 185418 B0.5 IIIn 0.42 2.54 V04 0.40 –10.7 ± 0.5 0.30 (σ)
HD 170740 B2 V 25 0.45 3.01 V04 0.58 –9.9 ± 1.5 0.26 (σ)
HD 147889 B2 V 100 1.03 3.95 V04 0.62 –6.7 ± 1.0 0.41 (ζ)
HD 169454e B1 Ia 49 1.03 3.37 V04 –9.9 ± 1.5 0.34 (σ)

Notes. (a) E(B–V) is based on photometry and intrinsic colors. (b)From Valencic et al. (2004; V04) and Wegner (2003; W03). (c)From Jenkins (2009). (d)The 5797/5780 DIB ratio is related to the effective UV radiation field strength; UV exposed environments, σ-type, have ratios <0.35, while UV-shielded, ζ-type environments, have ratios ≥0.35 (c.f. Vos et al. 2011). (e)HD 169454 is not a single-cloud line-of-sight but it is used for comparison (c.f. Sect. 7).

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