CWNU 1726

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0.39 UTI
0.34
CN
0.59
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 3.0 [N/pc2]
  • CN 0.34 Poorly populated
  • Cdens 0.59 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1726 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age 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– 233.08 -58.589 0.421 -3.218 -4.356 -42.309
Hunt & Reffert 2024 233.077 -58.596 0.409 -3.205 -4.371 12.409
Cavallo et al. 2024 233.1 -58.577 0.409 – – –
Hunt & Reffert 2023 233.077 -58.596 0.409 -3.205 -4.371 12.409
He et al. 2023 233.089 -58.595 0.422 -3.225 -4.354 -42.31

💡 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– 2.26 2.18 1.22 249 0.370 377 – –
Hunt & Reffert 2024 – – – – – 377(1) – –
Cavallo et al. 2024 2.39 2.18 – 135 0.370 – – –
Hunt & Reffert 2023 2.26 1.95 1.22 249 – – – –
He et al. 2023 2.24 2.20 – 398 – – – –

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

Visualization

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