CWNU 2664

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0.38 UTI
0.39
CN
0.28
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.4 [N/pc2]
  • CN 0.39 Poorly populated
  • Cdens 0.28 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2664 is a poorly populated, loose object of high 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– 190.823 -61.194 0.472 -4.894 -0.441 -23.574
Hunt & Reffert 2024 190.789 -61.166 0.466 -4.912 -0.486 -23.582
Cavallo et al. 2024 190.855 -61.183 0.465 – – –
Hunt & Reffert 2023 190.789 -61.166 0.466 -4.912 -0.486 -23.582
He et al. 2023 190.839 -61.187 0.469 -4.892 -0.46 –

💡 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 2.0 2.32 37 -0.280 268 – –
Hunt & Reffert 2024 – – – – – 268(1) – –
Cavallo et al. 2024 1.81 2.16 – 95 -0.280 – – –
Hunt & Reffert 2023 1.94 1.65 2.32 37 – – – –
He et al. 2023 2.00 2.00 – 20 – – – –

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

Visualization

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