CWNU 2357

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0.22 UTI
0.25
CN
0.12
Cdens
0.12
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 13.3 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.12 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2357 is a poorly populated, very loose object of very 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, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity Intermediate age

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 – 121.333 -35.877 0.604 -4.375 4.046 25.643
Hu & Soubiran 2025 121.351 -35.974 – – – –
Hunt & Reffert 2024 121.367 -36.016 0.596 -4.376 4.04 -6.702
Cavallo et al. 2024 121.351 -35.974 0.596 – – –
Hunt & Reffert 2023 121.367 -36.016 0.596 -4.376 4.04 -6.702
He et al. 2023 121.259 -35.873 0.602 -4.371 4.06 –

💡 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] Bfr BSS
Hu & Soubiran 2025 – – – – -0.200* – – –
Hunt & Reffert 2024 – – – – – 141* – –
Cavallo et al. 2024 1.63 1.65 – 525 0.230 – – –
Hunt & Reffert 2023 1.64 1.56 1.50 101 – – – –
He et al. 2023 1.58 2.10 – 251 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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