UPK 418

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0.26 UTI
0.0
CN
0.13
Cdens
0.25
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad) 0.7 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.13 Very loose
  • CC3 0.25 Low quality
  • Clit 0.45 Poorly studied
  • Cdup 1.0 Unique

Overview

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UPK 418 is a sparse, very loose object of low 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 absorption and age parameters (see Parameters). It is poorly studied in the literature.

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 112.565 5.58 1.017 -2.629 -1.112 36.308
Almeida et al. 2025 112.5 5.576 – – – –
Alfonso et al. 2024 112.615 5.705 1.14 -2.666 -1.555 –
Almeida et al. 2023 112.476 5.579 – – – –
Dias et al. 2021 112.5 5.576 1.116 -2.643 -1.146 –
Cantat-Gaudin et al. 2020 112.48 5.605 1.111 -2.646 -0.983 –
Cantat-Gaudin & Anders 2020 112.39 5.557 1.12 -2.651 -1.17 –
Sim et al. 2019 112.561 5.618 – -2.68 -1.6 –

💡 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– 0.87 0.06 – 89 -0.220 104 0.49 –
Almeida et al. 2025 0.87 0.20 – 197 – 76 – –
Alfonso et al. 2024 0.92 0.01 – 17 -0.220 – – –
Almeida et al. 2023 0.82 0.06 – 100 -0.068 131(1) 0.49 –
Tarricq et al. 2022 0.90 – – 63 – – – –
Dias et al. 2021 0.87 0.20 – 197 -0.220 – – –
Cantat-Gaudin et al. 2020 0.92 0.01 – 63 – – – –
Cantat-Gaudin & Anders 2020 0.87 – – – – – – –
Sim et al. 2019 0.83 – – 89 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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