UFMG 74

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0.65 UTI
0.75
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 31.2 [N/pc2]
  • CN 0.75 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 74 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, metal-poor, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.11 kpc) differs significantly from the median photometric distance (~1.74 kpc).

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

Cavallo et al. (2024)
Silver 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– 269.737 -20.586 0.322 -0.443 -1.809 19.897
Hunt & Reffert 2024 269.74 -20.583 0.324 -0.452 -1.829 5.471
Cavallo et al. 2024 269.728 -20.585 0.328 – – –
Hunt & Reffert 2023 269.74 -20.583 0.324 -0.452 -1.829 5.471
Ferreira et al. 2021 269.736 -20.588 0.289 -0.435 -1.785 –

💡 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– 1.74 4.45 2.93 145 -0.990 3015 – –
Hunt & Reffert 2024 – – – – – 3015(1) – –
Cavallo et al. 2024 1.71 4.60 – 145 -0.990 – – –
Hunt & Reffert 2023 2.75 4.45 2.93 54 – – – –
Ferreira et al. 2021 1.74 4.19 – 562 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0012 37.3 269.74 -20.59 0.32 -0.44 -1.82 19.9 0.0

💡 Note: The % column shows the percentage of members that UFMG 74 shares with each listed object.

Visualization

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