CWNU 124

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0.38 UTI
0.0
CN
1.0
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 8.9 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 124 is a sparse, very dense object of low C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, intermediate-age cluster (see Parameters). It is poorly studied 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– 349.188 64.718 1.001 0.626 -0.457 -33.512
Hunt & Reffert 2024 349.21 64.694 1.0 0.623 -0.443 -20.639
Cavallo et al. 2024 349.177 64.671 0.999 – – –
Hunt & Reffert 2023 349.21 64.694 1.0 0.623 -0.443 -20.639
He et al. 2022 349.121 64.689 1.0 0.63 -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– 1.04 2.1 0.48 162 0.545 87 – –
Hunt & Reffert 2024 – – – – – 87(1) – –
Cavallo et al. 2024 1.04 1.84 – 162 0.410 – – –
Hunt & Reffert 2023 1.03 2.10 0.48 230 – – – –
He et al. 2022 1.20 2.22 – 158 0.680 – – –

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

Visualization

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