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Table 3.

Spectral lines used for cross-correlation.

Star Rest wavelength
AS 314 Si II 4128–4130/He I 4471/Mg II 4481/Si II 6347-71
HD 160529 Si II 4128–4130/Mg II 4481
HD 168607 Si II 4128–4130/He I 4471/Mg II 4481/Si II 6347
HD 168625 He I 5876/Si II 6347-71/C II 6578-83
HD 316285 He I 4471/Mg II 4481/Fe II 4526-34-36/N II 5666-76-79-86/Al III 5723/S II 6449
HD 326823 N II 5666-76-79-86
MWC 314 S II 5454-74/Ne I 6402
MWC 930 He I 4471/Mg II 4481/N II 4630/Si III 4813-19-28
WR31a He I 4471/Mg II 4481/N II 4601-07-14-21-30/N II 5666-76-79-86
HD 80077 He I 4471/Mg II 4481/Si III 4552/N II 4601-07-14-21-30/Fe III 5156/N II 5666-76-79-86
WRAY 15–751 Mg II 4481/Si II 6347
HR Car N II 5666-76-79-86/Al III 5723
P Cyg S III 4253/Si III 4552/N II 4601-07-14-21-30/N II 5666-76-79-86
Sher 25 He I 4471/Mg II 4481/N II 5666-76-79-86/He I 5876
ζ Sco Si III 4813-19-28/N II 5666-76-79-86
Pistol Mg II 21,347-21,438
Schulte 12 N II 5666-76-79-86/He I 5876/Si II 6347
Cl* Westerlund 1 W 243 Si II 5979/Fe II 6179/Si II 6347-71

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