CWNU 379

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0.45 UTI
0.0
CN
0.88
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 3.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.88 Dense
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 379 is a sparse, dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.
Relatively close 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 – 214.082 -63.513 0.425 -4.956 -1.861 -20.315
Hu & Soubiran 2025 214.102 -63.51 – – – –
Hunt & Reffert 2024 214.103 -63.513 0.417 -4.961 -1.851 -11.754
Cavallo et al. 2024 214.102 -63.509 0.417 – – –
Hunt & Reffert 2023 214.103 -63.513 0.417 -4.961 -1.851 -11.754
He et al. 2022 214.064 -63.51 0.41 -4.99 -1.9 -28.4

💡 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 – – – – -0.220* – – –
Hunt & Reffert 2024 – – – – – 191* – –
Cavallo et al. 2024 1.99 1.09 – 1023 0.290 – – –
Hunt & Reffert 2023 2.18 1.30 0.51 318 – – – –
He et al. 2022 1.66 1.62 – 1259 -1.335 – – –

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

Visualization

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