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Erratum
This article is an erratum for:
[https://doi.org/10.1051/0004-6361/201732329]


Table 3

Radial velocities and equivalent widths (EWs) of the Ca II H&K and Na I D non-photospheric absorptions, radial velocities of the stars, and projected velocities of ISM clouds in the Colorado model.

Stars with non-photospheric absorptions

Star vCaIIK EW(K/H) ΔvCaIIK vNaID EW(D2/D1) (c) vrad vISM (d)
(km s−1) mÅ (km s−1) (km s−1) mÅ (km s−1) (km s−1)
HD 9672 (a) 13.5 ± 2.3 10.6/6.0 7.4 11.5 ± 2.3 16.4/9.3 11.0 ± 2.0 11.01 (LIC)
HD 32297 (a) 22.7 ± 3.0 19.4/8.9 9.7 23.8 ± 2.5 93.0/84.0 19.7 ± 2.0 23.59 (LIC)
HD 110058 (a) 12.7 ± 3.3 27.0/24.1 6.8 12.5 ± 2.8 46.0/39.1 12.6 ± 2.4 –14.46 (G)
1.2 ± 3.3 19.9/10.0 12.6 0.9 ± 2.8 34.0/18.9
HD 131488 (a) 4.0 ± 2.7 5.7/– 9.6 5.3 ± 2.2 42.1/34.2 5.8 ± 1.5 –23.91 (G)
–3.2 ± 2.7 4.0/– 4.2 –13.88 ± 2.2 7.2/–
HD 131835 (a) 2.2 ± 2.7 0.7/– 2.3 <0.9 2.6 ± 1.4 18.56 (GEM)
–5.9 ± 2.7 2.1/1.4 7.9 <0.9
–13.8 ± 2.7 8.3/4.1 7.4 –11.8 ± 2.0 41.0/32.1
HD 138813 –27.5 ± 3.0 5.6/– 18.7 –22.2 ± 2.2 5.9/3.1 –0.4 ± 2.0 –27.82 (G)
–12.0 ± 2.5 18.0/15.4
0.1 ± 2.0 –7.55/–5.2
HD 146897 –8.0 ± 2.7 12.4/– 7.2 –8.8 ± 2.1 118.2/80.0 –4.0 ± 1.5 –29.19 (G)
–30.0 ± 2.7 5.9/– 4.6 <0.8
HD 156623 (a) –15.0 ± 2.7 9.0/3.7 18.7 –1.8 ± 2.6 –10.6/–8.5 –0.2 ± 1.5 –24.89 (G)
8.1 ± 2.7 4.3/– 6.0 (e) <0.7
HD 172555 (a) 2.3 ± 3.0 9.9/4.0 9.7 15.3 ± 2.1 8.0/– 2.6 ± 1.9 –16.84 (G)
–20.4 ± 2.1 3.2/1.8
HD 181296 (b) –22.8 ± 3.8 3.9/2.2 8.4 –22.9 ± 2.4 4.0/– –3.0 ± 3.0 –18.51 (G)

Notes. The FWHM velocity dispersion of the Ca II K lines are also given. (a) Stars with FEBs or red wings. (b)The line of sight towards this star does not traverse any ISM cloud in the Colorado model but it passes within 20° of several clouds. Among these, cloud G is the closest one in velocity. (c) Upper limits are shown for those stars without Na non-photospheric absorption. (d) Names within brackets are ISM clouds in the Colorado model (Redfield & Linsky 2008). (e) The velocity dispersion for this absorption is highly variable, and the value shown here is the value obtained from the median spectra.

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