CWNU 6

Click to load Aladin Lite
0.22 UTI
0.25
CN
0.26
Cdens
0.38
CC3
0.1
Clit
1.0
Cdup
Core radius and density 1.2 [pc], 1.3 [pc-2]
  • CN 0.25 Poorly populated
  • Cdens 0.26 Loose
  • CC3 0.38 Low quality
  • Clit 0.1 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 6 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (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 open cluster. CMD class: 0.38 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.38 (50th percentile).

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 229.995 -56.188 0.588 -4.971 -3.002 -33.604
Hu & Soubiran 2025 229.987 -56.234 – – – –
Hunt & Reffert 2024 230.024 -56.192 0.565 -4.871 -2.983 -34.326
Cavallo et al. 2024 229.987 -56.234 0.578 – – –
Hunt & Reffert 2023 230.024 -56.192 0.565 -4.871 -2.983 -34.326
He et al. 2022 230.009 -56.214 0.6 -5.05 -3.01 -34.0

💡 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– 1.46 2.615 1.8 445 -0.100 222 – –
Hu & Soubiran 2025 – – – – -0.100(5) – – –
Hunt & Reffert 2024 1.63 2.81 1.80 96 – 222(1) – –
Cavallo et al. 2024 1.29 2.42 – 851 -0.650 – – –
Hunt & Reffert 2023 1.63 2.81 1.80 96 – – – –
He et al. 2022 1.26 1.90 – 794 0.161 – – –

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

Visualization

â„šī¸