CWNU 356

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0.57 UTI
0.52
CN
1.0
Cdens
0.75
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 10.6 [N/pc2]
  • CN 0.52 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 356 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the absorption and metallicity parameters (see Parameters). It is poorly studied in the literature.

Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 69 along with Theia_2166.

Palma et al. (2025)
Classified as tidal capture (resonant trapping pair) P205, along with Loden_1256.

Cavallo et al. (2024)
Silver 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– 215.066 -61.074 0.572 -3.704 -2.898 6.882
Hunt & Reffert 2024 215.058 -61.081 0.584 -3.673 -2.888 6.953
Cavallo et al. 2024 215.094 -61.057 0.585 – – –
Hunt & Reffert 2023 215.058 -61.081 0.584 -3.673 -2.888 6.953
He et al. 2022 215.061 -61.073 0.57 -3.71 -2.9 –

💡 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– 1.905 1.35 1.2 8 0.325 302 – –
Liu et al. 2025 2.94 0.53 – 9 – – – –
Hunt & Reffert 2024 – – – – – 302(1) – –
Cavallo et al. 2024 1.62 1.21 – 17 -0.030 – – –
Hunt & Reffert 2023 1.60 1.49 1.20 6 – – – –
He et al. 2022 2.19 1.80 – 5 0.680 – – –

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

Visualization

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