UBC 1031

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0.68 UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 3.1 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1031 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, old cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Relatively close High extinction Massive Near-solar metallicity Old

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 – 280.229 -9.667 0.394 0.738 -3.702 -24.165
Hu & Soubiran 2025 280.228 -9.693 – – – –
Hunt & Reffert 2024 280.226 -9.665 0.388 0.721 -3.666 -17.378
Cavallo et al. 2024 280.228 -9.693 0.391 – – –
Hunt & Reffert 2023 280.226 -9.665 0.388 0.721 -3.666 -17.378
Castro-Ginard et al. 2022 280.22 -9.67 0.4 0.74 -3.72 -25.02

💡 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] Bfr BSS
Hu & Soubiran 2025 – – – – 0.000* – – –
Hunt & Reffert 2024 – – – – – 1080* – –
Cavallo et al. 2024 2.27 3.64 – 1259 -0.270 – – –
Hunt & Reffert 2023 2.35 3.54 2.17 478 – – – –
Castro-Ginard et al. 2022 2.68 2.79 – 1239 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 404 96.7 280.23 -9.67 0.39 0.74 -3.7 -24.16 0.02
CWWDL 5705 49.2 280.22 -9.67 0.39 0.74 -3.7 -24.24 0.0

💡 Note: The % column shows the percentage of members that UBC 1031 shares with each listed object.

Visualization

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