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Table 6.
Results of searching for physically nearby stars to AM CVn stars.
| Gaia | RA | Dec | p | pmra | pmdec | G | g−r | Separation | |
|---|---|---|---|---|---|---|---|---|---|
| SourceID | J2000 | J2000 | (mas) | (mas yr−1) | (mas yr−1) | (mag) | (pc) | ||
| KL Dra | 2239471475135041664 | 291.159333 | 59.696233 | 1.04(15) | −2.46(30) | −18.27(26) | 19.05 | 1.21 | |
| 2239448930851818112 | 290.953649 | 59.610338 | 1.11(33) | −2.89(75) | −18.37(80) | 19.44 | 1.14 | 3.5 ± 0.6 | |
| SDSS J1525+3600 | 1375131155313563136 | 231.289887 | 36.015117 | 1.93(28) | 4.79(81) | −16.87(81) | 19.665 | 0.60 | |
| 1375135415921155968 | 231.150531 | 36.107433 | 1.63(60) | 5.25(129) | −16.410(129) | 20.226 | 1.13 | 1.4 ± 0.3 | |
| 1375131155313567232 | 231.288185 | 36.023225 | 2.28(15) | 5.24(28) | −14.492(28) | 18.293 | 1.20 | 0.06 ± 0.01 |
Notes. The candidate companion stars were selected by searching for stars within 3σ of the parallax to the AM CVn star and also 3σ of the proper motions in RA and Dec. In the final column we give the physical separation between the star and the AM CVn star.
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