CWNU 2347

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0.58 UTI
0.55
CN
1.0
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 1.4 [arcmin]
  • CN 0.55 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2347 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It was recently reported in the literature.
Distant Moderate extinction Near-solar metallicity Old

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 – 129.027 -48.146 0.197 -2.856 2.93 49.641
Hu & Soubiran 2025 129.019 -48.141 – – – –
Hunt & Reffert 2024 129.019 -48.143 0.191 -2.854 2.936 51.488
Cavallo et al. 2024 129.019 -48.141 0.191 – – –
Hunt & Reffert 2023 129.019 -48.143 0.191 -2.854 2.936 51.488
He et al. 2023 129.022 -48.145 0.198 -2.863 2.931 49.98

💡 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 – – – – -0.250* – – –
Hunt & Reffert 2024 – – – – – 701* – –
Cavallo et al. 2024 3.36 1.24 – 2138 -0.250 – – –
Hunt & Reffert 2023 4.69 1.37 1.75 1021 – – – –
He et al. 2023 4.37 1.45 – 794 – – – –

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

Visualization

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