UBC 1056

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0.57 UTI
0.36
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 10.3 [N/pc2]
  • CN 0.36 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1056 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age 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– 286.162 13.419 0.528 -0.269 -4.547 -5.671
Hunt & Reffert 2024 286.157 13.409 0.529 -0.278 -4.527 6.165
Cavallo et al. 2024 286.161 13.425 0.526 – – –
Hunt & Reffert 2023 286.157 13.409 0.529 -0.278 -4.527 6.165
Castro-Ginard et al. 2022 286.14 13.42 0.52 -0.27 -4.55 -5.47

💡 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– 2.08 2.84 2.22 263 0.350 325 – –
Hunt & Reffert 2024 – – – – – 325(1) – –
Cavallo et al. 2024 2.08 3.21 – 117 0.350 – – –
Hunt & Reffert 2023 1.78 2.84 2.22 263 – – – –
Castro-Ginard et al. 2022 2.12 2.19 – 349 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 235 69.4 286.16 13.41 0.53 -0.27 -4.58 -5.71 0.0

💡 Note: The % column shows the percentage of members that UBC 1056 shares with each listed object.

Visualization

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