UFMG 96

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0.63 UTI
0.66
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 6.3 [N/pc2]
  • CN 0.66 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
UFMG 96 is a moderately populated, 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, very metal-poor, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

Palma et al. (2025)
Classified as optical pair P500, along with HSC_2982.

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– 264.441 -29.772 0.421 -1.423 -3.382 -11.21
Hunt & Reffert 2024 264.423 -29.772 0.416 -1.397 -3.383 -23.062
Cavallo et al. 2024 264.448 -29.768 0.417 – – –
Hunt & Reffert 2023 264.423 -29.772 0.416 -1.397 -3.383 -23.062
Ferreira et al. 2021 264.455 -29.776 0.413 -1.442 -3.421 –

💡 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– 2.22 4.27 2.34 96 -1.530 1700 – –
Hunt & Reffert 2024 – – – – – 1700(1) – –
Cavallo et al. 2024 2.23 4.30 – 83 -1.530 – – –
Hunt & Reffert 2023 2.22 4.27 2.34 96 – – – –
Ferreira et al. 2021 1.51 3.97 – 355 – – – –

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

Visualization

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