UFMG 22

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0.69 UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad) 26.9 [N/pc2]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.35 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
UFMG 22 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, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.

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

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 263.197 -37.613 0.388 -0.355 -2.65 1.464
Almeida et al. 2025 263.199 -37.644 – – – –
Hunt & Reffert 2024 263.2 -37.612 0.403 -0.333 -2.646 33.779
Cavallo et al. 2024 263.186 -37.611 0.401 – – –
Hunt & Reffert 2023 263.2 -37.612 0.403 -0.333 -2.646 33.779
Dias et al. 2021 263.199 -37.644 0.364 -0.397 -2.605 –
Ferreira et al. 2020 263.19 -37.635 0.358 -0.412 -2.61 –

💡 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– 2.32 3.23 2.7 22 0.035 1044 – –
Almeida et al. 2025 2.33 3.23 – 12 – 623 – –
Hunt & Reffert 2024 – – – – – 1464(1) – –
Cavallo et al. 2024 2.00 4.10 – 28 -0.190 – – –
Hunt & Reffert 2023 2.32 3.66 2.70 22 – – – –
Dias et al. 2021 2.33 3.23 – 12 0.259 – – –
Ferreira et al. 2020 1.51 2.85 – 1000 – – – –

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

Visualization

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