UFMG 48

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0.63 UTI
0.68
CN
1.0
Cdens
0.75
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad) 10.0 [N/pc2]
  • CN 0.68 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.35 Poorly studied
  • Cdup 1.0 Unique

Overview

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UFMG 48 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is poorly studied in the literature.

Cavallo et al. (2024)
Gold sample.

Almeida et al. (2025)
Mass determination: good 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– 212.438 -59.324 0.357 -4.324 -1.849 –
Almeida et al. 2025 212.434 -59.341 – – – –
Hunt & Reffert 2024 212.429 -59.316 0.357 -4.309 -1.828 –
Cavallo et al. 2024 212.441 -59.321 0.357 – – –
Hunt & Reffert 2023 212.429 -59.316 0.357 -4.309 -1.828 –
Dias et al. 2021 212.434 -59.341 0.325 -4.312 -1.863 –
Ferreira et al. 2020 212.437 -59.356 0.321 -4.311 -1.866 –

💡 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– 2.68 2.62 2.77 265 0.250 587 – –
Almeida et al. 2025 2.68 2.62 – 265 – 480 – –
Hunt & Reffert 2024 – – – – – 694(1) – –
Cavallo et al. 2024 2.19 2.12 – 417 0.510 – – –
Hunt & Reffert 2023 2.52 2.57 2.77 50 – – – –
Dias et al. 2021 2.68 2.62 – 265 -0.010 – – –
Ferreira et al. 2020 3.02 3.41 – 224 – – – –

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

Visualization

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