UFMG 47

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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) 20.2 [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 47 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, intermediate-age cluster, but with a large variance across recent sources for the age parameter (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)
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 99999– 253.024 -47.396 0.343 0.016 -2.085 -26.444
Almeida et al. 2025 253.022 -47.395 – – – –
Hunt & Reffert 2024 253.033 -47.391 0.349 0.025 -2.096 -35.07
Cavallo et al. 2024 253.023 -47.397 0.348 – – –
Hunt & Reffert 2023 253.033 -47.391 0.349 0.025 -2.096 -35.07
Dias et al. 2021 253.022 -47.395 0.326 -0.04 -2.079 –
Ferreira et al. 2020 253.02 -47.399 0.323 -0.071 -2.073 –

💡 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– 2.56 3.95 1.98 269 0.262 1002 – –
Almeida et al. 2025 2.33 3.25 – 468 – 509 – –
Hunt & Reffert 2024 – – – – – 1494(1) – –
Cavallo et al. 2024 2.70 4.23 – 269 0.180 – – –
Hunt & Reffert 2023 2.56 3.95 1.98 115 – – – –
Dias et al. 2021 2.33 3.25 – 468 0.344 – – –
Ferreira et al. 2020 2.63 4.50 – 178 – – – –

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

Visualization

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