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Table 4.

Radial velocities listed for photospheric lines, the He I narrow emission component, and for each of the Gaussian components of the Hα profile decomposition (see text).

Photosphere
He I
Hα
EW
HJD Vr σVr Vr σVr Vem Vblue Vred Hα Hβ Hγ He I (NC)




(2 450 000+) (km s−1) (km s−1) (km s−1) (Å)
8054.90048 17.1 0.3 8.8 0.4 −28.3 −75.4 −13.8 10.7 4.3 3.1 0.14
8055.89091 17.2 0.3 4.3 0.4 −16.0 −75.0 −12.9 11.2 4.4 3.5 0.17
8057.00939 17.2 0.2 5.7 0.4 −18.3 −42.6 −2.5 9.1 3.1 2.2 0.17
8057.99515 16.8 0.3 8.4 0.4 −16.9 −33.6 −0.9 12.2 5.0 3.6 0.21
8059.05448 17.0 0.3 8.8 0.3 −31.6 −55.2 1.6 13.2 5.0 3.3 0.19
8060.95421 17.4 0.2 2.5 0.4 −27.3 −34.4 0.8 11.7 3.7 2.5 0.18
8061.95085 16.9 0.3 5.8 0.3 −20.9 −32.5 3.6 9.9 3.6 3.0 0.24
8063.08059 17.8 0.3 8.9 0.3 −18.7 −67.1 −9.1 14.2 5.2 3.8 0.2
8064.99530 17.3 0.2 3.0 0.5 −10.3 −48.1 −4.8 5.2 1.7 1.5 0.15
8065.99958 17.1 0.3 5.5 0.4 6.7 −45.0 −7.8 4.5 2.0 1.4 0.17
8066.91484 16.2 0.3 9.0 0.3 −25.1 −55.7 −7.6 6.2 2.9 3.0 0.21

Notes. The EWs are also listed for Balmer lines and the He I narrow component.

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