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Table 4

Means of radial velocities of stellar Balmer lines Hγ, Hδ, Hϵ, and H8, of the shell absorption in Hα, and of other stellar lines (He I 4026, He I 4143, He I 4471, and Mg II 4481).

Spectrogr. HJD-2400000 Radial velocity
Hγ-H8 Shell Hα Other

(d) (km s−1)
C 46085.621 37.5
C 46085.681 38.8
C 46086.647 34.6
C 46086.793 35.8
H 49861.975 33.8 34.5 30.7
H 50160.065 44.6 34.5 45.9
H 50172.030 42.9 31.4 46.5
H 50220.962 38.5 32.8 35.9
H 50224.964 33.4 33.1 33.8
H 50227.943 32.7
H 50228.443 34.5 31.7
H 50230.957 34.2 33.2 29.4
H 50236.952 33.5 32.1 29.5
H 50238.953 32.8
H 50456.077 40.1 33.7 26.2
H 50467.193 34.7
H 50471.181 36.6 34.5 27.9
H 50477.171 36.1 32.8 28.2
H 50516.011 34.9 33.9 24.0
H 50531.059 36.2 33.4 29.0
H 50551.041 33.8 35.0 29.8
F 51183.230 32.9 31.8: 32.1
H 51299.959 30.6 36.2: 26.3
H 51311.004 29.1 35.4: 20.2
H 51328.976 31.4 37.6: 19.6
H 51341.955 35.5 37.3:
H 51352.951 32.4
F 51382.446 29.3 32.8 32.6
F 51384.440 31.4 31.9 30.6
F 51564.289 34.0 30.3
F 53396.999 30.9 28.1
F 53397.000 30.2 25.4
F 53398.001 29.4 29.4
E 57411.391 33.7 31.0

Notes. For a description of the measurement procedures see Sect. 3.1. C, E, F, and H identify the spectrographs used: CES, ESPaDOns, FEROS, and HEROS, respectively. The ESPaDOns entry is the average over 40 spectra obtained within less than 1 h. The CES measurements are from Baade (1989a) and are based on He I 4471.5 and Mg II 4481.2 only. After ∼HJD 2451500, emission or shell absorption components of Hα were no longer visible. Colons (:) indicate uncertain measurements.

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