CWNU 2079

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0.14 UTI
0.0
CN
0.15
Cdens
0.38
CC3
0.1
Clit
1.0
Cdup
Core radius and density 2.0 [pc], 0.8 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.15 Very loose
  • CC3 0.38 Low quality
  • Clit 0.1 Rarely studied
  • Cdup 1.0 Unique

Overview

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CWNU 2079 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Cavallo et al. (2024)
Gold sample.

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– 54.361 52.477 0.514 -1.764 -0.756 -75.718
Hu & Soubiran 2025 54.23 52.44 – – – –
Hunt & Reffert 2024 54.385 52.479 0.516 -1.712 -0.741 -83.27
Cavallo et al. 2024 54.23 52.44 0.513 – – –
Hunt & Reffert 2023 54.385 52.479 0.516 -1.712 -0.741 -83.27
He et al. 2023 54.364 52.461 0.514 -1.779 -0.715 -75.34

💡 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– 1.92 3.65 2.31 920 0.000 260 – –
Hu & Soubiran 2025 – – – – 0.040(5) – – –
Hunt & Reffert 2024 1.89 3.65 2.31 920 – 260(1) – –
Cavallo et al. 2024 1.95 3.39 – 912 -0.040 – – –
Hunt & Reffert 2023 1.89 3.65 2.31 920 – – – –
He et al. 2023 1.95 3.70 – 1413 – – – –

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

Visualization

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