Table A.3.
RR Lyrae stars presenting a proper motion anomaly.
Name | Period | ϖ | μHG (mas a−1) | μHip − μHG (mas a−1) | ΔHip | μG2 − μHG (mas a−1) | ΔG2 | PM | RR | |||
---|---|---|---|---|---|---|---|---|---|---|---|---|
(d) | (mas) | μα | μδ | μα | μδ | μα | μδ | bin. | ||||
SW And | 0.44 | 1.81 | −6.56 0.04 | −18.83 0.03 | −0.30 1.33 | +1.25 0.88 | 1.4 | −0.20 0.14 | −0.56 0.26 | 2.6 | ° | AB |
XX And | 0.72 | 0.72 | +58.31 0.04 | −32.84 0.05 | +1.36 1.50 | −1.34 1.31 | 1.4 | −0.31 0.11 | −0.13 0.12 | 3.0 | • | AB |
AT And | 0.62 | 2.21 | −8.62 0.03 | −50.81 0.05 | +0.46 1.28 | +0.19 1.39 | 0.4 | −7.09 0.45 | −2.15 0.39 | 16.7 † ‡ | ⋆ | AB |
WY Ant | 0.57 | 0.94 | +35.91 0.04 | −50.19 0.05 | +0.43 1.57 | +0.72 1.53 | 0.5 | +0.50 0.17 | +0.01 0.15 | 2.9 | ° | AB |
DN Aqr | 0.63 | 0.67 | +46.81 0.07 | −15.34 0.06 | +3.94 2.79 | +3.32 1.73 | 2.4 | −0.09 0.13 | −0.20 0.12 | 1.8 | ° | AB |
… | … | … | … | … | … | … | … | … | …… | … | … | … |
Notes. Columns are identical to Table A.1, except “RR” lists the subtype of variability. When the Arenou et al. (2018) quality control parameters are not all satisfied, the star is marked with † after ΔG2, and when RUWE 𝜚 > 1.4 they are marked with ‡ (Sect. 2.3). The complete table is available at the CDS.
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