CWNU 1093

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0.20 UTI
0.35
CN
0.06
Cdens
0.38
CC3
0.1
Clit
1.0
Cdup
Core radius and density 2.0 [pc], 0.3 [pc-2]
  • CN 0.35 Poorly populated
  • Cdens 0.06 Very loose
  • CC3 0.38 Low quality
  • Clit 0.1 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1093 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age 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.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.24 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.24 (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– 117.18 20.2 1.842 -6.881 -4.278 18.631
Yang et al. 2025 117.26 20.179 – – – –
Zhang et al. 2024 117.26 20.179 – – – –
Cavallo et al. 2024 116.827 20.426 1.812 – – –
Hunt & Reffert 2023 117.26 20.179 1.799 -6.956 -4.375 16.622
He et al. 2022 117.061 20.281 1.844 -6.906 -4.299 –

💡 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– 0.54 0.09 0.65 242 -0.101 – – –
Yang et al. 2025 – – – 240 -0.210(3) – – –
Zhang et al. 2024 – – – – -0.101(1) – – –
Cavallo et al. 2024 0.55 0.32 – 251 0.170 – – –
Hunt & Reffert 2023 0.53 0.09 0.65 243 – – – –
He et al. 2022 – 0.05 – 89 – – – –

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

Visualization

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