UFMG 90

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0.64 UTI
0.71
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.5 [arcmin]
  • CN 0.71 Moderately 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 90 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, very metal-poor, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~2.18 kpc) differs significantly from the median photometric distance (~1.60 kpc).

Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.

Relatively close High extinction Massive Very metal-poor Intermediate age

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 – 270.637 -25.819 0.458 0.558 -0.02 -48.969
Hunt & Reffert 2024 270.64 -25.816 0.471 0.588 0.008 -38.703
Cavallo et al. 2024 270.644 -25.818 0.474 – – –
Hunt & Reffert 2023 270.64 -25.816 0.471 0.588 0.008 -38.703
Ferreira et al. 2021 270.655 -25.83 0.44 0.455 -0.083 –

💡 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 – – – – – 1668* – –
Cavallo et al. 2024 1.60 4.30 – 263 -1.010 – – –
Hunt & Reffert 2023 2.01 3.87 2.75 147 – – – –
Ferreira et al. 2021 1.48 3.56 – 794 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2859 28.3 270.64 -25.81 0.46 0.59 -0.02 -48.4 0.0

💡 Note: The % column shows the percentage of members that UFMG 90 shares with each listed object.

Visualization

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