CWNU 331

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0.40 UTI
0.32
CN
0.81
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 4.1 [N/pc2]
  • CN 0.32 Poorly populated
  • Cdens 0.81 Dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 331 is a poorly populated, dense object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the metallicity parameter (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– 124.435 -39.543 0.819 -5.05 4.187 12.125
Hunt & Reffert 2024 124.471 -39.521 0.826 -5.051 4.151 11.991
Cavallo et al. 2024 124.457 -39.591 0.825 – – –
Hunt & Reffert 2023 124.471 -39.521 0.826 -5.051 4.151 11.991
He et al. 2022 124.421 -39.567 0.83 -5.05 4.16 –

💡 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– 1.39 1.68 1.15 10 0.456 125 – –
Hunt & Reffert 2024 – – – – – 125(1) – –
Cavallo et al. 2024 1.39 1.68 – 8 0.050 – – –
Hunt & Reffert 2023 1.14 1.35 1.15 15 – – – –
He et al. 2022 1.86 2.22 – 10 0.862 – – –

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

Visualization

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