CWNU 222

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0.12 UTI
0.0
CN
0.35
Cdens
0.12
CC3
0.06
Clit
1.0
Cdup
Core radius and density 0.8 [pc], 1.8 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.35 Loose
  • CC3 0.12 Very low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 222 is a sparse, loose object of very low C3 quality. Its parallax locates it at a relatively close distance, below 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 open cluster. CMD class: 1.00 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (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– 101.999 -8.04 0.621 -1.944 -0.84 23.401
Hunt & Reffert 2024 101.993 -8.019 0.624 -1.943 -0.787 25.617
Cavallo et al. 2024 102.048 -8.123 0.615 – – –
Hunt & Reffert 2023 101.993 -8.019 0.624 -1.943 -0.787 25.617
He et al. 2022 101.986 -8.039 0.62 -1.93 -0.84 –

💡 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– 1.52 0.93 0.22 212 -0.190 147 – –
Hunt & Reffert 2024 1.52 0.93 0.22 167 – 147(1) – –
Cavallo et al. 2024 1.59 0.88 – 257 0.200 – – –
Hunt & Reffert 2023 1.52 0.93 0.22 167 – – – –
He et al. 2022 1.32 1.27 – 501 -0.580 – – –

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

Visualization

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