UBC 452

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0.37 UTI
0.33
CN
0.16
Cdens
0.5
CC3
0.44
Clit
1.0
Cdup
Radius (P>50% members) 5.8 [arcmin]
  • CN 0.33 Poorly populated
  • Cdens 0.16 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.44 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 452 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Distant Low extinction Near-solar metallicity Intermediate age

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 – 111.183 -19.257 0.266 -1.297 0.672 68.423
Li et al. 2025 111.185 -19.225 0.258 -1.327 0.652 –
Hu & Soubiran 2025 111.186 -19.255 – – – –
Hunt & Reffert 2024 111.196 -19.259 0.267 -1.293 0.672 71.086
Cavallo et al. 2024 111.186 -19.255 0.268 – – –
Hunt & Reffert 2023 111.196 -19.259 0.267 -1.293 0.672 71.086
Cantat-Gaudin et al. 2020 111.185 -19.225 0.258 -1.327 0.652 –
Castro-Ginard et al. 2020 111.18 -19.237 0.257 -1.325 0.64 –

💡 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 1.79 0.38 – 795 -0.108 – – –
Hu & Soubiran 2025 – – – – -0.250* – – –
Hunt & Reffert 2024 – – – – – 205* – –
Cavallo et al. 2024 2.81 1.23 – 646 0.000 – – –
Hunt & Reffert 2023 3.53 1.20 0.95 406 – – – –
Cantat-Gaudin et al. 2020 3.39 0.70 – 1000 – – – –

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

Visualization

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