UFMG 61

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0.40 UTI
0.0
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 11.6 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UFMG 61 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age 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– 185.471 -63.633 0.455 -4.239 -0.163 -19.571
Hunt & Reffert 2024 185.462 -63.628 0.456 -4.237 -0.17 -9.142
Cavallo et al. 2024 185.442 -63.631 0.456 – – –
Hunt & Reffert 2023 185.462 -63.628 0.456 -4.237 -0.17 -9.142
Ferreira et al. 2020 185.555 -63.61 0.395 -4.208 -0.248 –

💡 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– 2.01 0.94 0.88 122 0.260 258 – –
Hunt & Reffert 2024 – – – – – 258(1) – –
Cavallo et al. 2024 1.85 0.89 – 380 0.260 – – –
Hunt & Reffert 2023 2.01 0.94 0.88 122 – – – –
Ferreira et al. 2020 2.46 1.71 – 71 – – – –

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

Visualization

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