UFMG 47

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0.70 UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members) 2.9 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.38 Poorly studied
  • Cdup 1.0 Unique

Overview

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 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.

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 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] Bfr BSS
Almeida et al. 2025 2.33 3.25 468 509
Hunt & Reffert 2024 1494*
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

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.
(*): indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

Galactocentric position diagram

💡 Note: How are the galactocentric plots generated? See FAQ.