UFMG 42

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0.61 UTI
0.79
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 46.6 [N/pc2]
  • CN 0.79 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UFMG 42 is a rich, very dense object of 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.

Cavallo et al. (2024)
Wood 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– 236.042 -55.251 0.368 -6.081 -4.399 -63.27
Hunt & Reffert 2024 236.038 -55.249 0.381 -6.037 -4.408 -60.185
Cavallo et al. 2024 236.038 -55.283 0.375 – – –
Hunt & Reffert 2023 236.038 -55.249 0.381 -6.037 -4.408 -60.185
Ferreira et al. 2020 236.04 -55.251 0.32 -6.289 -4.235 –

💡 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– 2.67 5.79 2.89 288 0.000 2709 – –
Hunt & Reffert 2024 – – – – – 2709(1) – –
Cavallo et al. 2024 2.67 5.26 – 288 0.000 – – –
Hunt & Reffert 2023 2.48 5.79 2.89 376 – – – –
Ferreira et al. 2020 5.01 6.82 – 89 – – – –

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

Visualization

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