CWNU 1666

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0.20 UTI
0.32
CN
0.07
Cdens
0.5
CC3
0.06
Clit
1.0
Cdup
Core radius and density 4.2 [pc], 0.3 [pc-2]
  • CN 0.32 Poorly populated
  • Cdens 0.07 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1666 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, young 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.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD classes: 0.99 (50th percentile), true positive (human-assigned).

Hunt & Reffert (2023)
Classified as open cluster. CMD classes: 0.99 (50th percentile), true positive (human-assigned).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 94.364 4.945 0.439 -0.242 -2.004 22.405
Hunt & Reffert 2024 94.313 5.013 0.433 -0.243 -1.957 22.366
Cavallo et al. 2024 94.378 4.944 0.431 – – –
Hunt & Reffert 2023 94.313 5.013 0.433 -0.243 -1.957 22.366
He et al. 2023 94.381 4.943 0.442 -0.254 -2.004 –

💡 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– 2.13 1.715 1.01 95 0.360 210 – –
Hunt & Reffert 2024 2.13 1.65 1.01 95 – 210(1) – –
Cavallo et al. 2024 2.28 1.78 – 115 0.360 – – –
Hunt & Reffert 2023 2.13 1.65 1.01 95 – – – –
He et al. 2023 2.09 2.00 – 40 – – – –

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

Visualization

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