Table 7
Candidate stars of the kinematic groups in the sample of K–M dwarfs.
| MCC | HIP | d | U | V | W | e | Z max | Δυ | ΔD0 | Notes |
| (pc) | (km s-1) | (km s-1) | (km s-1) | (pc) | (km s-1) | (pc) | ||||
|
|
||||||||||
| β Pictoris Moving Group | ||||||||||
| MCC 392A | 11437 | 40 | –13.6 ± 0.9 | –15.0 ± 0.4 | –8.2 ± 0.6 | 0.015 ± 0.003 | 14 ± 2 | 3.7 | 18 | M(2) |
| MCC 392B | 40 | –11.1 ± 1.6 | –14.0 ± 1.6 | –7.5 ± 1.7 | 0.007 ± 0.008 | 11 ± 1 | 2.7 | 43 | M(2) | |
| MCC 111 | 23200 | 26 | –12.4 ± 0.3 | –16.9 ± 0.4 | –9.6 ± 0.2 | 0.019 ± 0.003 | 23 ± 3 | 2.5 | 19 | M(1) |
| MCC 824 | 102409 | 10 | –10.1 ± 0.2 | –16.4 ± 0.2 | –10.4 ± 0.1 | 0.017 ± 0.003 | 30 ± 3 | 1.3 | 23 | M(2) |
| ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... |
Notes. This table is available at the CDS. A portion of the first page of the table is shown here for guidance regarding its form and content. Description of columns: Cols. 1, 2: MCC number or Hipparcos number (for stars from the CNS list); Col. 3: distance from the Sun, in pc; Cols. 4–6: heliocentric velocity components and their errors; Col. 7: orbital eccentricity and its error; Col. 8: orbital distance Zmax and its error; Col. 9: difference Δυ between the total velocity of the star and the velocity of the SKG; Col. 10: distance ΔD0 from the center of SKG at the time of SKG’s birth; Col. 11: notes on SKG membership from the literature (M – probable/possible member, NM – nonmember, with the source indicated in parentheses).
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