CWNU 1471

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0.27 UTI
0.28
CN
0.47
Cdens
0.12
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 2.3 [N/pc2]
  • CN 0.28 Poorly populated
  • Cdens 0.47 Loose
  • CC3 0.12 Very low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1471 is a poorly populated, loose object of very low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young 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– 90.215 25.877 0.488 0.583 -2.034 –
Hunt & Reffert 2024 90.286 25.951 0.488 0.594 -2.021 –
Cavallo et al. 2024 90.208 25.913 0.49 – – –
Hunt & Reffert 2023 90.286 25.951 0.488 0.594 -2.021 –
He et al. 2023 90.205 25.868 0.488 0.583 -2.036 –

💡 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 1.27 0.64 62 -0.080 105 – –
Hunt & Reffert 2024 – – – – – 105(1) – –
Cavallo et al. 2024 1.87 1.21 – 62 -0.080 – – –
Hunt & Reffert 2023 1.94 1.27 0.64 78 – – – –
He et al. 2023 2.04 1.60 – 28 – – – –

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

Visualization

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