CWNU 2431

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0.29 UTI
0.0
CN
0.21
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.1 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.21 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2431 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

Palma et al. (2025)
Classified as optical pair P351, along with Hogg_17.

Cavallo et al. (2024)
Silver 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– 219.34 -60.97 0.417 -4.64 -3.219 -38.926
Hunt & Reffert 2024 219.377 -60.959 0.415 -4.623 -3.214 -38.881
Cavallo et al. 2024 219.356 -60.962 0.413 – – –
Hunt & Reffert 2023 219.377 -60.959 0.415 -4.623 -3.214 -38.881
He et al. 2023 219.244 -60.982 0.422 -4.631 -3.217 –

💡 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– 2.24 1.47 1.89 14 0.960 253 – –
Hunt & Reffert 2024 – – – – – 253(1) – –
Cavallo et al. 2024 2.26 1.00 – 85 0.960 – – –
Hunt & Reffert 2023 2.19 1.47 1.89 14 – – – –
He et al. 2023 2.24 1.70 – 11 – – – –

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

Visualization

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