CWNU 119

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0.09 UTI
0.0
CN
0.22
Cdens
0.12
CC3
0.06
Clit
1.0
Cdup
Core radius and density 1.3 [pc], 1.1 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.22 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 119 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is rarely studied 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)
Part of multiple system G104, along with King_6 and HSC_1146.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.98 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.98 (50th percentile).

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 47.433 57.926 1.36 0.915 -5.061 -6.872
Hunt & Reffert 2024 47.45 57.934 1.354 0.886 -5.034 -4.376
Cavallo et al. 2024 47.154 57.952 1.355 – – –
Hunt & Reffert 2023 47.45 57.934 1.354 0.886 -5.034 -4.376
He et al. 2022 47.456 57.938 1.36 0.91 -5.06 –

💡 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– 0.705 1.95 0.98 57 0.317 43 – –
Hunt & Reffert 2024 0.70 1.95 0.98 57 – 43(1) – –
Cavallo et al. 2024 0.82 1.93 – 32 0.560 – – –
Hunt & Reffert 2023 0.70 1.95 0.98 57 – – – –
He et al. 2022 0.71 2.09 – 158 0.073 – – –

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

Visualization

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