CWNU 1922

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0.22 UTI
0.0
CN
0.73
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 3.7 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.73 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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CWNU 1922 is a sparse, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as an intermediate-age cluster (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.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 257.051 -42.464 0.443 -0.98 -4.125 -73.474
Hunt & Reffert 2024 257.048 -42.465 0.454 -0.968 -4.146 -59.904
Hunt & Reffert 2023 257.048 -42.465 0.454 -0.968 -4.146 -59.904
He et al. 2023 257.042 -42.456 0.454 -1.005 -4.145 -74.11

💡 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– 2.095 3.465 1.84 798 – 390 – –
Hunt & Reffert 2024 – – – – – 390(1) – –
Hunt & Reffert 2023 2.10 3.53 1.84 596 – – – –
He et al. 2023 2.09 3.40 – 1000 – – – –

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

Visualization

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