Table A.1
RVs of the primary determined from different spectral lines.
spectral ID | He Iλ3819 (a) | He Iλ3935 | He IIλ4025 (b) | N IVλ4058 | He IIλ4200 | mean value(c) |
---|---|---|---|---|---|---|
[km s−1] | [km s−1] | [km s−1] | [km s−1] | [km s−1] | [km s−1] | |
5 | 114 ± 63 | 117 ± 22 | 120 ± 8 | 103 ± 7 | 105 ± 4 | 112 ± 14 |
6 | — | 229 ± 26 | 236 ± 8 | 217 ± 21 | 210 ± 4 | 223 ± 9 |
7 | 48 ± 63 | 36 ± 47 | 53 ± 8 | 46 ± 9 | 55 ± 8 | 47 ± 16 |
8 | 140 ± 13 | 115 ± 34 | 134 ± 11 | 117 ± 18 | 122 ± 4 | 126 ± 8 |
9 | 145 ± 59 | — | 153 ± 10 | 134 ± 22 | 131 ± 5 | 141 ± 16 |
10 | 201 ± 53 | 215 ± 25 | 209 ± 11 | 195 ± 18 | 183 ± 8 | 201 ± 13 |
11 | 223 ± 32 | 212 ± 26 | 214 ± 9 | 192 ± 13 | 196 ± 4 | 207 ± 9 |
12 | 162 ± 18 | 167 ± 32 | 131 ± 14 | 137 ± 45 | 144 ± 8 | 148 ± 12 |
(a)The He I λ3819 is present in the primary and secondary spectrum. We note that the observed He I λ3819 line also contains the He II λ3813 line from the primary. (b)The He II λ4025 line has a strong contribution from the secondary. (c) The mean value is calculated as where RVi is the RV of line i and n is the total number of lines used. The errors of the mean values are calculated via Gaussian error propagation.
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