UPK 137

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0.56 UTI
0.33
CN
0.61
Cdens
0.75
CC3
0.55
Clit
1.0
Cdup
Radius (P>50% members) 13.3 [arcmin]
  • CN 0.33 Poorly populated
  • Cdens 0.61 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.55 Moderately studied
  • Cdup 1.0 Unique

Overview

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UPK 137 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is moderately studied in the literature.
Close Low extinction Near-solar metallicity Young

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

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 306.028 54.102 1.174 -2.292 -6.083 -17.255
Almeida et al. 2025 305.995 54.114 – – – –
Alfonso et al. 2024 305.981 54.381 1.13 -2.613 -6.119 –
Cavallo et al. 2024 306.076 54.195 1.175 – – –
Hunt & Reffert 2023 306.272 54.391 1.175 -2.312 -6.08 -13.364
Dias et al. 2021 305.995 54.114 1.155 -2.31 -6.061 –
Cantat-Gaudin et al. 2020 306.015 54.152 1.166 -2.289 -6.064 –
Cantat-Gaudin & Anders 2020 305.97 54.131 1.165 -2.297 -6.006 –
Sim et al. 2019 305.978 54.161 – -2.34 -6.04 –

💡 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 0.83 0.39 – 171 – 70 – –
Alfonso et al. 2024 0.81 0.35 – 90 0.006 – – –
Cavallo et al. 2024 0.86 0.38 – 79 0.490 – – –
Hunt & Reffert 2023 0.82 0.17 0.44 86 – – – –
Tarricq et al. 2022 0.83 – – 63 – – – –
Dias et al. 2021 0.83 0.39 – 171 0.006 – – –
Cantat-Gaudin et al. 2020 0.81 0.35 – 51 – – – –
Cantat-Gaudin & Anders 2020 0.84 – – – – – – –
Sim et al. 2019 0.84 – – 32 – – – –

Visualization

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