UBC 131

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0.00 UTI
0.31
CN
0.75
Cdens
1.0
CC3
0.0
Clit
0.0
Cdup
Radius (P>50% members) 10.5 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 0.75 Dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
UBC 131 is a poorly populated, dense object of very high C3 quality. Its parallax locates it at a close distance, below the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 6 years.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

No fundamental parameters

Castro-Ginard et al. (2020)
Coincidence with Sim et al. (2019, J. Korean Astron. Soc., 52, 145) or Liu & Pang (2019ApJS..245...32L), see Sect. 4.1.5.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 310.179 20.068 1.065 -6.259 -9.286 24.318
Castro-Ginard et al. 2020 310.236 20.152 1.068 -6.257 -9.215 –

💡 Note: The UCC values are estimated from its identified members.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Alessi 116 100.0 310.21 20.16 1.08 -6.29 -9.3 24.38 0.66
CWWDL 14281 100.0 310.2 20.17 1.07 -6.28 -9.3 23.99 0.0
UPK 84 100.0 310.22 20.21 1.08 -6.29 -9.29 24.19 0.3

💡 Note: The % column shows the percentage of members that UBC 131 shares with each listed object.

Visualization

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