CWNU 350

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0.29 UTI
0.0
CN
0.29
Cdens
0.38
CC3
0.4
Clit
1.0
Cdup
Stellar density (N50/rad) 1.5 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.29 Loose
  • CC3 0.38 Low quality
  • Clit 0.4 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 350 is a sparse, loose object of low C3 quality. Its parallax locates it at a relatively 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, age, and metallicity parameters (see Parameters). It is poorly studied in the literature.

Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 3 along with ASCC_13.

Palma et al. (2025)
Part of multiple system G8, along with HSC_1292 and ASCC_13.

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 99999– 76.425 45.993 0.903 -0.549 -1.768 -34.29
Hu & Soubiran 2025 76.476 45.943 – – – –
Zhang et al. 2024 76.466 45.969 – – – –
Hunt & Reffert 2024 76.466 45.969 0.904 -0.504 -1.757 -22.79
Cavallo et al. 2024 76.476 45.943 0.904 – – –
Hunt & Reffert 2023 76.466 45.969 0.904 -0.504 -1.757 -22.79
He et al. 2022 76.361 46.033 0.94 -0.55 -1.74 –

💡 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– 1.055 0.86 0.9 96 -0.093 102 – –
Liu et al. 2025 1.10 0.19 – 112 – – – –
Hu & Soubiran 2025 – – – – -0.230(5) – – –
Zhang et al. 2024 – – – – -0.126(1) – – –
Hunt & Reffert 2024 – – – – – 102(1) – –
Cavallo et al. 2024 1.06 1.09 – 1549 -0.060 – – –
Hunt & Reffert 2023 1.05 0.70 0.90 33 – – – –
He et al. 2022 1.05 1.02 – 79 0.370 – – –

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

Visualization

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