CWNU 2211

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0.21 UTI
0.25
CN
0.15
Cdens
0.5
CC3
0.06
Clit
1.0
Cdup
Core radius and density 2.3 [pc], 0.7 [pc-2]
  • CN 0.25 Poorly populated
  • Cdens 0.15 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 2211 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, below 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 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)
Part of multiple system G133, along with UBC_1376, HSC_1847 and HSC_1848.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.93 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.93 (50th percentile).

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 108.922 -19.561 0.332 -2.587 1.518 –
Hunt & Reffert 2024 108.93 -19.576 0.325 -2.585 1.494 –
Cavallo et al. 2024 108.936 -19.573 0.328 – – –
Hunt & Reffert 2023 108.93 -19.576 0.325 -2.585 1.494 –
He et al. 2023 108.919 -19.565 0.348 -2.587 1.525 –

💡 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– 2.835 1.61 1.98 282 0.270 338 – –
Hunt & Reffert 2024 2.79 1.61 1.98 283 – 338(1) – –
Cavallo et al. 2024 2.88 1.56 – 490 0.270 – – –
Hunt & Reffert 2023 2.79 1.61 1.98 282 – – – –
He et al. 2023 2.88 2.00 – 22 – – – –

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

Visualization

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