CWNU 1502

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0.40 UTI
0.26
CN
0.78
Cdens
0.38
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 3.9 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 0.78 Dense
  • CC3 0.38 Low quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1502 is a poorly populated, dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, intermediate-age cluster, but with a large variance across recent sources for the age parameter (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– 350.893 60.636 0.247 -3.255 -1.556 –
Hu & Soubiran 2025 350.866 60.632 – – – –
Hunt & Reffert 2024 350.892 60.625 0.249 -3.246 -1.538 –
Cavallo et al. 2024 350.866 60.632 0.244 – – –
Hunt & Reffert 2023 350.892 60.625 0.249 -3.246 -1.538 –
He et al. 2023 350.878 60.638 0.262 -3.256 -1.557 –

💡 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– 3.47 2.8 2.01 178 0.590 414 – –
Hunt & Reffert 2024 – – – – – 414(1) – –
Cavallo et al. 2024 3.31 2.24 – 513 0.590 – – –
Hunt & Reffert 2023 3.72 2.81 2.01 48 – – – –
He et al. 2023 3.47 2.80 – 178 – – – –

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

Visualization

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