UBC 590

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0.60 UTI
0.25
CN
1.0
Cdens
0.75
CC3
0.5
Clit
1.0
Cdup
Radius (P>50% members) 1.5 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.5 Moderately studied
  • Cdup 1.0 Unique

Overview

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UBC 590 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is moderately studied in the literature.
Distant High extinction Near-solar metallicity Very young

Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit. Silver sample.

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 – 313.824 47.566 0.239 -3.105 -4.135 –
Almeida et al. 2025 313.83 47.579 – – – –
Hunt & Reffert 2024 313.842 47.56 0.242 -3.076 -4.138 –
Celli et al. 2024 313.824 47.579 – – – –
Cavallo et al. 2024 313.839 47.539 0.241 – – –
Hunt & Reffert 2023 313.842 47.56 0.242 -3.076 -4.138 –
Dias et al. 2021 313.83 47.579 0.224 -3.112 -4.11 –
Cantat-Gaudin et al. 2020 313.824 47.579 0.222 -3.134 -4.102 –
Castro-Ginard et al. 2020 313.797 47.599 0.221 -3.137 -4.14 –

💡 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
Almeida et al. 2025 4.35 3.20 – 5 – 223 – –
Hunt & Reffert 2024 – – – – – 388* – –
Celli et al. 2024 – – – 12 – 260 – –
Cavallo et al. 2024 3.10 3.10 – 251 0.350 – – –
Hunt & Reffert 2023 4.04 3.61 1.00 13 – – – –
Dias et al. 2021 4.35 3.20 – 5 0.324 – – –
Cantat-Gaudin et al. 2020 3.80 3.37 – 12 – – – –

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

Visualization

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