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Table 3.

Properties and observed tangential velocity anomaly ΔvT, G2 for the 17 white dwarfs of our sample.

Name m1 ΔvT, G2 ΔG2 Δ
(M) (m s−1) (MJ au−1/2)
Wolf 28 0.680.02 11.05.2 2.1 °
LAWD 37 0.610.01 14.12.9 4.9
CPD-69 177 0.680.02 5.78.6 0.7
LAWD 74 0.620.02 7.111.6 0.6
DN Dra 0.750.03 13.49.7 1.4
CD-38 10980 0.680.02 15.014.1 1.1
HD 340611 0.640.03 26.111.7 2.2 °
GD 140 0.970.03 53.716.1 3.3
BD-07 3632 0.530.08 31.019.3 1.6
CD-30 17706 0.610.02 7.414.6 0.5
GD 279 0.640.03 41.815.1 2.8 °
LAWD 23 0.690.03 37.647.1 0.8
HIP 117059 0.560.05 29.674.4 0.4
EGGR 141 0.620.02 21.821.3 1.0
EGGR 150 0.630.02 27.726.3 1.1
LAWD 52 0.580.01 28.022.8 1.2
Feige 22 0.590.02 37.735.1 1.1

Notes. The estimated mass of the WD is listed in the m1 column, ΔG2 is the signal-to-noise ratio of the PMa and is the normalized mass of the companion (or an upper limit). The column Δ is set to • for 3 <  ΔG2 <  5 and ° for 2 <  ΔG2 <  3.

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