UBC 391

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0.58 UTI
0.26
CN
0.75
Cdens
1.0
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad) 3.7 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 0.75 Dense
  • CC3 1.0 Very high quality
  • Clit 0.45 Poorly 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 poorly studied in the literature.

Palma et al. (2025)
Classified as optical pair P603, along with UBC_389.

Cavallo et al. (2024)
Gold sample.

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 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] Bfrac BSS
UCC 99999– 2.335 2.78 1.19 55 0.156 273 – –
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(1) – –
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 – – – –

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

Visualization

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