CWNU 466

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0.23 UTI
0.0
CN
0.3
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 13.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.3 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 466 is a sparse, loose object of low C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It is poorly 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.

Relatively close Moderate extinction Metal-rich Young

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 36.414 64.303 1.066 -0.739 0.906 -23.514
Hunt & Reffert 2024 36.329 64.343 1.068 -0.748 0.876 -29.765
Cavallo et al. 2024 36.527 64.3 1.066 – – –
Hunt & Reffert 2023 36.329 64.343 1.068 -0.748 0.876 -29.765
He et al. 2022 36.44 64.307 1.02 -0.77 0.91 –

💡 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] Bfr BSS
Hunt & Reffert 2024 – – – – – 71* – –
Cavallo et al. 2024 1.07 2.54 – 35 0.110 – – –
Hunt & Reffert 2023 0.90 2.30 1.02 90 – – – –
He et al. 2022 1.00 1.86 – 631 0.916 – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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