CWNU 2063

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0.18 UTI
0.27
CN
0.05
Cdens
0.38
CC3
0.1
Clit
1.0
Cdup
Core radius and density 1.1 [pc], 0.2 [pc-2]
  • CN 0.27 Poorly populated
  • Cdens 0.05 Very loose
  • CC3 0.38 Low quality
  • Clit 0.1 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 2063 is a poorly populated, very loose object of low 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, intermediate-age cluster, but with a large variance across recent sources for the age parameter (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 class: 0.95 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.95 (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– 86.749 24.748 0.26 0.478 -0.655 -7.376
Zhang et al. 2024 86.694 24.746 – – – –
Hunt & Reffert 2024 86.694 24.746 0.25 0.494 -0.641 –
Cavallo et al. 2024 86.736 24.747 0.253 – – –
Hunt & Reffert 2023 86.694 24.746 0.25 0.494 -0.641 –
He et al. 2023 86.755 24.765 0.268 0.473 -0.672 –

💡 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– 3.96 2.32 1.39 235 -0.110 255 – –
Zhang et al. 2024 – – – – -0.049(1) – – –
Hunt & Reffert 2024 3.83 2.20 1.39 353 – 255(1) – –
Cavallo et al. 2024 4.09 2.44 – 117 -0.170 – – –
Hunt & Reffert 2023 3.83 2.20 1.39 353 – – – –
He et al. 2023 4.57 3.05 – 9 – – – –

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

Visualization

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