CWNU 472

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0.20 UTI
0.0
CN
0.14
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 12.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.14 Very loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 472 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a significant percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

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 Intermediate age

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 – 96.661 -8.327 0.626 -0.069 -1.01 4.02
Hunt & Reffert 2024 96.637 -8.296 0.635 -0.074 -1.028 4.026
Cavallo et al. 2024 96.613 -8.274 0.633 – – –
Hunt & Reffert 2023 96.637 -8.296 0.635 -0.074 -1.028 4.026
He et al. 2022 96.677 -8.388 0.6 0.02 -0.66 –

💡 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 – – – – – 68* – –
Cavallo et al. 2024 1.68 1.44 – 417 0.360 – – –
Hunt & Reffert 2023 1.51 1.47 1.49 136 – – – –
He et al. 2022 2.34 1.62 – 631 0.916 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 143 72.0 96.56 -8.17 0.63 -0.05 -1.03 4.02 0.18

💡 Note: The % column shows the percentage of members that CWNU 472 shares with each listed object.

Visualization

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