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Table 3

Summary of variability properties of the centroid velocity v and EW for 12 spectral lines of HD 188209 available in the HERMES data, spanning 1800 d.

Spectral Laboratory Colour Minimum Maximum Range Average Minimum Maximum Range
Line Wavelength (Å)1 Code v (km s-1) v (km s-1) v (km s-1) v (km s-1) EW (Å) EW (Å) EW (Å)

Hα 6562.801 light green –292.4 +439.6 732.0 –85.6 –0.163 0.694 0.857
Hγ 4340.464 light blue –42.4 –23.9 18.5 –34.4 1.353 1.553 0.201
Hβ 4861.325 black –41.4 –17.2 24.2 –31.7 1.249 1.631 0.382
Si iii 4567.841 purple –24.1 +1.7 25.8 –14.4 0.094 0.137 0.044
He i 4922.931 cyan –18.9 +1.9 20.8 –10.6 0.495 0.589 0.094
He i 5875.599 grey –21.6 +5.4 27.1 –10.2 0.987 1.378 0.391
He i 5015.678 pink –18.8 +4.3 23.1 –10.0 0.328 0.391 0.063
He i 4713.139 dark blue –17.5 +0.2 17.7 –9.4 0.325 0.410 0.085
He ii 5410.53 yellow –16.2 –1.3 14.9 –9.2 0.363 0.398 0.035
He ii 4541.591 green –13.3 +3.9 17.3 –7.6 0.220 0.311 0.091
C iv 5811.97 orange –11.9 +4.4 16.3 –5.5 0.085 0.107 0.022
He ii 4685.71 red +8.8 +43.7 34.8 20.8 0.187 0.253 0.066

Notes. Systematic uncertainties in the average values of v are different for the different spectral lines and may amount to several km s-1 per spectral line. This is typically an order of magnitude larger than the statistical uncertainties for each of the v-values for a fixed spectral line.

(1)

Retrieved from the Atomic Line List available at http://www.pa.uky.edu/~peter/newpage/.

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