CWNU 1579

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0.22 UTI
0.39
CN
0.09
Cdens
0.38
CC3
0.12
Clit
1.0
Cdup
Core radius and density 3.9 [pc], 0.5 [pc-2]
  • CN 0.39 Poorly populated
  • Cdens 0.09 Very loose
  • CC3 0.38 Low quality
  • Clit 0.12 Rarely studied
  • Cdup 1.0 Unique

Overview

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CWNU 1579 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, young cluster, but with a large variance across recent sources for the age parameter (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.

Palma et al. (2025)
Classified as optical pair P319, along with HSC_2324.

Cavallo et al. (2024)
Silver sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.20 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.20 (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– 153.878 -57.09 0.401 -5.971 3.908 –
Hunt & Reffert 2024 153.851 -57.077 0.392 -6.0 3.906 –
Cavallo et al. 2024 154.072 -57.223 0.396 – – –
Hunt & Reffert 2023 153.851 -57.077 0.392 -6.0 3.906 –
He et al. 2023 153.871 -57.103 0.406 -5.967 3.906 –

💡 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– 2.32 1.54 2.4 81 0.780 192 – –
Hunt & Reffert 2024 2.32 1.30 2.40 81 – 192(1) – –
Cavallo et al. 2024 2.67 1.78 – 65 0.780 – – –
Hunt & Reffert 2023 2.32 1.30 2.40 81 – – – –
He et al. 2023 2.24 2.95 – 282 – – – –

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

Visualization

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