UPK 526

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0.38 UTI
0.0
CN
0.17
Cdens
0.75
CC3
0.5
Clit
1.0
Cdup
Stellar density (N50/rad) 0.8 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.17 Very loose
  • CC3 0.75 High quality
  • Clit 0.5 Moderately studied
  • Cdup 1.0 Unique

Overview

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UPK 526 is a sparse, very loose object of high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is moderately studied in the literature.

Almeida et al. (2025)
Mass determination: worst 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 99999– 115.351 -52.81 1.746 -7.985 7.449 19.483
Li et al. 2025 115.198 -52.839 1.712 -8.0 7.415 –
Almeida et al. 2025 115.268 -52.91 – – – –
Alfonso et al. 2024 114.395 -52.836 1.727 -7.84 7.688 –
Cavallo et al. 2024 113.782 -52.946 1.755 – – –
Hunt & Reffert 2023 115.946 -52.836 1.75 -7.774 7.804 14.398
Dias et al. 2021 115.268 -52.91 1.722 -8.006 7.434 23.348
Cantat-Gaudin et al. 2020 115.198 -52.839 1.712 -8.0 7.415 –
Cantat-Gaudin & Anders 2020 115.274 -52.829 1.727 -8.006 7.464 –
Sim et al. 2019 115.237 -52.774 – -7.98 7.42 –

💡 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– 0.57 0.47 0.99 25 -0.030 74 – –
Li et al. 2025 0.55 0.47 – 21 -0.066 – – –
Almeida et al. 2025 0.56 0.58 – 38 – 74 – –
Alfonso et al. 2024 0.63 0.45 – 20 -0.030 – – –
Cavallo et al. 2024 0.61 0.68 – 14 0.080 – – –
Hunt & Reffert 2023 0.54 0.46 0.99 29 – – – –
Dias et al. 2021 0.56 0.58 – 38 -0.030 – – –
Cantat-Gaudin et al. 2020 0.63 0.45 – 31 – – – –
Cantat-Gaudin & Anders 2020 0.57 – – – – – – –
Sim et al. 2019 0.57 – – 20 – – – –

Visualization

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