UFMG 63

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0.55 UTI
0.5
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 5.1 [arcmin]
  • CN 0.5 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

UFMG 63 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 263.373 -25.016 0.805 1.227 -0.276 -12.001
Hunt & Reffert 2024 263.383 -25.011 0.797 1.193 -0.257 4.238
Cavallo et al. 2024 263.356 -25.038 0.799
Hunt & Reffert 2023 263.383 -25.011 0.797 1.193 -0.257 4.238
Ferreira et al. 2021 263.4 -25.01 0.805 1.231 -0.279

💡 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
Hunt & Reffert 2024 444*
Cavallo et al. 2024 1.03 4.03 170 -0.200
Hunt & Reffert 2023 1.18 3.83 1.89 126
Ferreira et al. 2021 1.00 4.34 63

💡 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.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0002 84.3 263.36 -25.01 0.81 1.23 -0.26 -12.0 0.02

💡 Note: The % column shows the percentage of members that UFMG 63 shares with each listed object.

Visualization

Galactocentric position diagram

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