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Table 1

Binary systems found from common parallaxes and proper motions, with at least a UCD candidate in their components.

Name Spectral type RA deg Dec deg μRA mas yr−1 μDec mas yr−1 Parallax mas
2MASS J23495194-2627594(a) M5.0 357.4676880 −26.4661806 237.744 72.853 23.274
J2349-2627 L2.5 357.4723326 −26.4647437 237.085 73.130 21.905

2MASS 07215434-3104365 M3.0 110.4767231 −31.0778963 52.475 −227.870 41.1380
J0721-3105 M6.5 110.4802981 −31.0885526 57.029 −229.768 41.048

J0943-2009 M7.5 145.8666910 −20.1648161 −221.041 180.053 19.937
J0943-2010 M8.5 145.8661622 −20.1676840 −219.376 179.819 19.932

Gaia DR2 4757030391786232576 WD 82.3906350 −63.9487136 166.109 −4.879 14.048
J0529-6357 M7.5 82.4196342 −63.9525915 165.976 −3.968 14.122

J0945-4120 M8.0 146.3288956 −41.3450184 −144.533 83.965 17.139
2MASS 09450332-4115209 M5? 146.2629519 −41.2554272 −145.015 84.615 17.357

J1456-5059 M8.5 224.1588143 −50.9860720 −419.117 −128.584 31.110
2MASS 14563857-5059174 M3? 224.1576894 −50.9887596 −420.868 −146.202 30.799

J0347+0417 M8 56.7820854 4.2981726 113.323 −49.331 30.928(b)
Gaia DR3 3271777035212786944 M9.5? 56.7820761 4.2983795 121.010 −45.425 31.00

Notes. “?” denotes an unconfirmed spectral type, issued from photometric relations of Reylé (2018) or Hawley et al. (2002). (a)Identified in the RAVE survey (RAVE DR6, Steinmetz et al. 2020) as a 0.10 M, 9 Gyr star, with a radial velocity of 12.00 ± 3.85 km s−1.(b) Analysed as a spectral binary, see Sect. 4.4.

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