Table A.1
HERMES and CORAVEL radial velocities for components of some visual binaries lacking velocities so far.
JD−2 400 000 | Vr(A) | Vr(B) | HER/COR | Note |
|
||||
WDS 09006+4147AB | ||||
55 520.795 | 29.06 ± 0.09 | 22.06 ± 0.08 | H | a |
55 521.640 | 29.03 ± 0.10 | 21.93 ± 0.09 | H | – |
55 579.783 | 29.44 ± 0.09 | 21.83 ± 0.08 | H | – |
55 589.620 | 29.53 ± 0.09 | 21.68 ± 0.08 | H | – |
55 647.599 | 29.64 ± 0.08 | 21.45 ± 0.07 | H | – |
56 046.402 | 31.11 ± 0.09 | 19.92 ± 0.05 | H | – |
56 244.717 | 31.54 ± 0.13 | 19.48 ± 0.07 | H | – |
WDS 09144+5241A | ||||
56 039.412 | 10.620 ± 0.002 | – | H | – |
WDS 09144+5241B | ||||
56 039.418 | – | 11.848 ± 0.002 | H | – |
WDS 10454+3831AB | ||||
56 040.468 | −3.380 ± 0.003 | – | H | – |
56 040.485 | – | −3.175 ± 0.005 | H | b |
WDS 13491+2659AB | ||||
45 441.525 | −20.32 ± 0.32 | – | C | – |
45 475.401 | −19.29 ± 0.45 | −22.70 ± 0.42 | C | – |
45 789.537 | −20.27 ± 0.33 | −23.18 ± 0.37 | C | – |
46 214.395 | −20.06 ± 0.32 | −23.95 ± 0.35 | C | – |
46 562.422 | −20.48 ± 0.31 | −23.80 ± 0.37 | C | – |
51 018.433 | −20.27 ± 0.44 | −23.01 ± 0.46 | C | – |
WDS 17153-2636A | ||||
56 038.716 | 0.532 ± 0.002 | – | H | – |
WDS 17153-2636B | ||||
56 038.719 | – | 0.246 ± 0.001 | H | – |
WDS 17364+6820Aa,Ab | ||||
55 6038.682 | −30.0 ± 0.3 | −27.0 ± 0.5 | H | c |
WDS 18428+5938AB | ||||
55 655.719 | −1.061 ± 0.006 | – | H | – |
55 660.748 | −1.048 ± 0.005 | – | H | – |
56 037.736 | −1.074 ± 0.005 | – | H | – |
56 038.695 | −1.088 ± 0.005 | – | H | – |
56 038.699 | – | 0.779 ± 0.006 | H | – |
WDS 19255+0307Aa,Ab | ||||
55 657.742 | −28.68 ± 0.26 | −37.70 ± 0.09 | H |
Notes. The quoted error corresponds to the fitting error, but does not account for the pressure-driven zero-point shift, which can amount up to 200 m s-1 for HERMES velocities (Raskin et al. 2011). a: Component A (V = 4.2), of spectral type F4V, is a fast rotator. It has the largest peak on the HERMES cross-correlation function (Fig. A.5). For details see note in Appendix A; b: barely separable; c: “blind” assignment based on the depth of the cross-correlation peak: component A is assumed to have the deeper peak.
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