UFMG 95

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0.56 UTI
0.3
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 5.6 [arcmin]
  • CN 0.3 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 95 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a very metal-poor, young cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It is poorly studied in the literature.
Relatively close Low extinction Very metal-poor Young

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 – 270.695 -29.377 0.849 1.808 -0.952 -19.872
Hunt & Reffert 2024 270.688 -29.384 0.845 1.797 -1.017 -17.399
Cavallo et al. 2024 270.665 -29.384 0.845 – – –
Hunt & Reffert 2023 270.688 -29.384 0.845 1.797 -1.017 -17.399
Ferreira et al. 2021 270.695 -29.37 0.839 1.815 -0.895 –

💡 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] Bfr BSS
Hunt & Reffert 2024 – – – – – 227* – –
Cavallo et al. 2024 0.89 1.24 – 35 -1.160 – – –
Hunt & Reffert 2023 1.13 0.25 0.41 57 – – – –
Ferreira et al. 2021 1.00 0.46 – 158 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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