UFMG 54

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0.66 UTI
0.81
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 52.0 [N/pc2]
  • CN 0.81 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UFMG 54 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

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

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– 210.687 -61.956 0.292 -7.651 -2.154 -36.716
Hunt & Reffert 2024 210.679 -61.96 0.269 -7.658 -2.159 -36.745
Cavallo et al. 2024 210.657 -61.966 0.269 – – –
Hunt & Reffert 2023 210.679 -61.96 0.269 -7.658 -2.159 -36.745
Ferreira et al. 2020 210.717 -61.976 0.274 -7.633 -2.069 –

💡 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– 3.8 5.77 2.59 309 0.350 1464 – –
Hunt & Reffert 2024 – – – – – 1464(1) – –
Cavallo et al. 2024 3.80 5.20 – 309 0.350 – – –
Hunt & Reffert 2023 3.09 5.77 2.59 453 – – – –
Ferreira et al. 2020 3.80 7.19 – 40 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 2629 9.2 210.69 -61.96 0.36 -7.67 -2.14 -36.75 0.0

💡 Note: The % column shows the percentage of members that UFMG 54 shares with each listed object.

Visualization

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