UFMG 53

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0.56 UTI
0.35
CN
1.0
Cdens
0.75
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad) 5.5 [N/pc2]
  • CN 0.35 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.35 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
UFMG 53 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high 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.

Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.

Cavallo et al. (2024)
Bronze 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– 195.47 -64.043 0.334 -8.805 -0.904 -24.756
Almeida et al. 2025 195.425 -64.034 – – – –
Hunt & Reffert 2024 195.497 -64.04 0.321 -8.793 -0.941 -15.844
Cavallo et al. 2024 195.455 -64.027 0.32 – – –
Hunt & Reffert 2023 195.497 -64.04 0.321 -8.793 -0.941 -15.844
Dias et al. 2021 195.425 -64.034 0.336 -8.724 -0.916 –
Ferreira et al. 2020 195.41 -64.03 0.343 -8.707 -0.925 –

💡 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– 2.89 3.11 2.09 57 -0.122 344 – –
Almeida et al. 2025 2.89 3.11 – 14 – 305 – –
Hunt & Reffert 2024 – – – – – 382(1) – –
Cavallo et al. 2024 4.88 3.01 – 380 -0.410 – – –
Hunt & Reffert 2023 2.91 3.89 2.09 57 – – – –
Dias et al. 2021 2.89 3.11 – 14 0.165 – – –
Ferreira et al. 2020 2.75 4.19 – 251 – – – –

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

Visualization

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