CWNU 1399

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0.58 UTI
0.52
CN
1.0
Cdens
0.75
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 25.0 [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 1399 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, old 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– 182.184 -62.594 0.196 -8.341 1.361 -30.742
Hu & Soubiran 2025 182.192 -62.597 – – – –
Hunt & Reffert 2024 182.187 -62.594 0.189 -8.341 1.349 -28.17
Cavallo et al. 2024 182.192 -62.597 0.195 – – –
Hunt & Reffert 2023 182.187 -62.594 0.189 -8.341 1.349 -28.17
He et al. 2023 182.186 -62.597 0.209 -8.344 1.361 -30.74

💡 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– 4.69 3.86 1.98 1122 -0.390 2610 – –
Hu & Soubiran 2025 – – – – -0.440(5) – – –
Hunt & Reffert 2024 – – – – – 2610(1) – –
Cavallo et al. 2024 5.01 3.86 – 1000 -0.340 – – –
Hunt & Reffert 2023 4.69 3.64 1.98 1679 – – – –
He et al. 2023 3.89 4.05 – 1122 – – – –

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

Visualization

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