CWNU 2379

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0.25 UTI
0.0
CN
0.44
Cdens
0.75
CC3
0.03
Clit
1.0
Cdup
Core radius and density 1.1 [pc], 2.2 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.44 Loose
  • CC3 0.75 High quality
  • Clit 0.03 Rarely studied
  • Cdup 1.0 Unique

Overview

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CWNU 2379 is a sparse, loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a 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)
Part of multiple system G183, along with UBC_93 and HSC_56.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.42 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.42 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 269.134 -25.629 0.321 -0.477 -1.481 –
Hunt & Reffert 2024 269.138 -25.635 0.319 -0.461 -1.492 –
Hunt & Reffert 2023 269.138 -25.635 0.319 -0.461 -1.492 –
He et al. 2023 269.136 -25.631 0.316 -0.466 -1.496 –

💡 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– 3.11 4.32 2.15 55 – 760 – –
Hunt & Reffert 2024 3.11 4.32 2.15 55 – 760(1) – –
Hunt & Reffert 2023 3.11 4.32 2.15 55 – – – –
He et al. 2023 3.63 5.20 – 5 – – – –

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

Visualization

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