UFMG 71

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0.56 UTI
0.32
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 5.9 [N/pc2]
  • CN 0.32 Poorly populated
  • 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 71 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, young cluster (see Parameters). It is poorly studied in the literature.

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– 265.557 -27.335 0.651 0.712 -1.788 –
Hunt & Reffert 2024 265.553 -27.336 0.654 0.744 -1.784 –
Cavallo et al. 2024 265.589 -27.333 0.655 – – –
Hunt & Reffert 2023 265.553 -27.336 0.654 0.744 -1.784 –
Ferreira et al. 2021 265.555 -27.329 0.603 0.764 -1.777 –

💡 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– 1.26 2.94 0.7 52 -0.970 308 – –
Hunt & Reffert 2024 – – – – – 308(1) – –
Cavallo et al. 2024 1.10 3.16 – 38 -0.970 – – –
Hunt & Reffert 2023 1.44 2.47 0.70 52 – – – –
Ferreira et al. 2021 1.26 2.94 – 100 – – – –

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

Visualization

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