UBC 632

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0.43 UTI
0.0
CN
0.32
Cdens
0.75
CC3
0.55
Clit
1.0
Cdup
Radius (P>50% members) 3.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.32 Loose
  • CC3 0.75 High quality
  • Clit 0.55 Moderately studied
  • Cdup 1.0 Unique

Overview

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UBC 632 is a sparse, loose object of high C3 quality. Its parallax locates it at a moderate distance, well above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the absorption and age parameters (see Parameters). It is moderately studied in the literature.
Distant Low extinction Near-solar metallicity Old

Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit.

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 – 121.6 -9.622 0.25 -2.549 1.806 –
Li et al. 2025 121.59 -9.602 0.264 -2.471 1.729 –
Hu & Soubiran 2025 121.602 -9.614 – – – –
Almeida et al. 2025 121.589 -9.606 – – – –
Hunt & Reffert 2024 121.587 -9.64 0.271 -2.561 1.809 –
Cavallo et al. 2024 121.602 -9.614 0.268 – – –
Hunt & Reffert 2023 121.587 -9.64 0.271 -2.561 1.809 –
Dias et al. 2021 121.589 -9.606 0.315 -2.476 1.721 –
Cantat-Gaudin et al. 2020 121.59 -9.602 0.264 -2.471 1.729 –
Castro-Ginard et al. 2020 121.598 -9.588 0.274 -2.459 1.747 –

💡 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
Li et al. 2025 3.82 0.34 – 1611 -0.234 – – –
Hu & Soubiran 2025 – – – – -0.180* – – –
Almeida et al. 2025 4.11 1.51 – 49 – 355 – –
Hunt & Reffert 2024 – – – – – 169* – –
Cavallo et al. 2024 2.79 0.13 – 2042 -0.130 – – –
Hunt & Reffert 2023 3.45 0.04 0.15 1199 – – – –
Dias et al. 2021 4.11 1.51 – 49 -0.254 – – –

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

Visualization

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