CWNU 1382

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0.43 UTI
0.34
CN
0.93
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 4.7 [N/pc2]
  • CN 0.34 Poorly populated
  • Cdens 0.93 Very dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1382 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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– 46.313 55.912 0.377 -0.336 -0.03 32.938
Hunt & Reffert 2024 46.326 55.897 0.39 -0.343 -0.022 13.458
Cavallo et al. 2024 46.317 55.91 0.388 – – –
Hunt & Reffert 2023 46.326 55.897 0.39 -0.343 -0.022 13.458
He et al. 2023 46.315 55.909 0.38 -0.315 -0.032 -52.09

💡 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– 2.43 4.32 2.15 170 0.340 536 – –
Hunt & Reffert 2024 – – – – – 536(1) – –
Cavallo et al. 2024 2.64 4.25 – 170 0.340 – – –
Hunt & Reffert 2023 2.43 4.32 2.15 163 – – – –
He et al. 2023 2.34 4.65 – 178 – – – –

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

Visualization

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