UBC 114

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0.67 UTI
0.57
CN
1.0
Cdens
1.0
CC3
0.4
Clit
1.0
Cdup
Stellar density (N50/rad) 10.1 [N/pc2]
  • CN 0.57 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.4 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 114 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 286.421 -0.396 0.647 -1.466 -1.915 24.077
Li et al. 2025 286.446 -0.399 0.656 -1.47 -1.874 –
Hunt & Reffert 2024 286.425 -0.394 0.64 -1.484 -1.949 15.597
Cavallo et al. 2024 286.422 -0.398 0.645 – – –
Hunt & Reffert 2023 286.425 -0.394 0.64 -1.484 -1.949 15.597
Tarricq et al. 2022 286.353 -0.389 0.663 -1.464 -1.921 –
Cantat-Gaudin et al. 2020 286.446 -0.399 0.656 -1.47 -1.874 –
Castro-Ginard et al. 2020 286.44 -0.407 0.661 -1.495 -1.88 –

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

Reference Year Dist [kpc] Av [mag] DAv [mag] Age [Myr] [Fe/H] [dex] Mass [Msun] Bfrac BSS
UCC 99999– 1.47 1.275 1.27 56 0.102 454 – –
Li et al. 2025 1.34 1.27 – 36 0.043 – – –
Hunt & Reffert 2024 – – – – – 454(1) – –
Cavallo et al. 2024 1.48 1.28 – 62 0.160 – – –
Hunt & Reffert 2023 1.46 1.38 1.27 56 – – – –
Tarricq et al. 2022 1.47 – – 56 – – – –
Cantat-Gaudin et al. 2020 1.52 1.02 – 50 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14117 59.4 286.41 -0.41 0.66 -1.47 -1.96 24.08 0.06

💡 Note: The % column shows the percentage of members that UBC 114 shares with each listed object.

Visualization

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