CWNU 1473

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0.22 UTI
0.0
CN
0.38
Cdens
0.12
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 1.9 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.38 Loose
  • CC3 0.12 Very low quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1473 is a sparse, loose object of very low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (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– 98.069 9.6 0.474 -1.051 -0.227 –
Hu & Soubiran 2025 98.082 9.565 – – – –
Hunt & Reffert 2024 98.087 9.602 0.465 -1.053 -0.233 –
Cavallo et al. 2024 98.082 9.564 0.473 – – –
Hunt & Reffert 2023 98.087 9.602 0.465 -1.053 -0.233 –
He et al. 2023 98.084 9.591 0.48 -1.066 -0.226 –

💡 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– 1.94 0.86 1.09 119 0.015 125 – –
Hu & Soubiran 2025 – – – – -0.230(5) – – –
Hunt & Reffert 2024 – – – – – 125(1) – –
Cavallo et al. 2024 1.96 0.51 – 631 0.260 – – –
Hunt & Reffert 2023 1.94 0.86 1.09 119 – – – –
He et al. 2023 1.82 1.10 – 45 – – – –

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

Visualization

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