UBC 391

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0.60 UTI
0.26
CN
0.75
Cdens
1.0
CC3
0.5
Clit
1.0
Cdup
Radius (P>50% members) 3.6 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 0.75 Dense
  • CC3 1.0 Very high quality
  • Clit 0.5 Moderately studied
  • Cdup 1.0 Unique

Overview

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UBC 391 is a poorly populated, dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is moderately studied in the literature.
Relatively close Moderate extinction Near-solar metallicity Young

Almeida et al. (2025)
Mass determination: intermediate 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 – 338.947 59.057 0.397 -2.807 -2.009 –
Li et al. 2025 338.939 59.051 0.393 -2.859 -2.004 –
Almeida et al. 2025 338.894 59.007 – – – –
Hunt & Reffert 2024 338.956 59.054 0.407 -2.786 -2.005 –
Cavallo et al. 2024 338.927 59.045 0.405 – – –
Hunt & Reffert 2023 338.956 59.054 0.407 -2.786 -2.005 –
Dias et al. 2021 338.894 59.007 0.369 -2.827 -1.984 -72.75
Cantat-Gaudin et al. 2020 338.939 59.051 0.393 -2.859 -2.004 –
Castro-Ginard et al. 2020 338.841 59.043 0.397 -2.84 -2.004 –

💡 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 2.34 2.81 – 529 -0.041 – – –
Almeida et al. 2025 2.39 2.75 – 12 – 339 – –
Hunt & Reffert 2024 – – – – – 207* – –
Cavallo et al. 2024 2.11 2.91 – 100 0.530 – – –
Hunt & Reffert 2023 2.33 3.03 1.19 60 – – – –
Dias et al. 2021 2.39 2.75 – 12 0.156 – – –
Cantat-Gaudin et al. 2020 2.32 2.38 – 50 – – – –

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

Visualization

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