CWNU 2160

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0.20 UTI
0.0
CN
0.13
Cdens
0.75
CC3
0.06
Clit
1.0
Cdup
Core radius and density 1.7 [pc], 0.6 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.13 Very loose
  • CC3 0.75 High quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 2160 is a sparse, very loose object of high C3 quality. Its parallax locates it at a large distance, well above the mid-plane, affected by high extinction. It is catalogued as a very metal-poor, 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)
Silver sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.02 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.02 (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– 307.111 48.916 0.16 -2.538 -3.805 -62.876
Hunt & Reffert 2024 307.111 48.907 0.145 -2.527 -3.805 -62.857
Cavallo et al. 2024 307.115 48.916 0.138 – – –
Hunt & Reffert 2023 307.111 48.907 0.145 -2.527 -3.805 -62.857
He et al. 2023 307.117 48.901 0.14 -2.549 -3.823 -62.01

💡 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– 6.49 3.09 1.76 401 -1.340 498 – –
Hunt & Reffert 2024 7.61 3.09 1.76 199 – 498(1) – –
Cavallo et al. 2024 3.28 3.64 – 603 -1.340 – – –
Hunt & Reffert 2023 7.61 3.09 1.76 199 – – – –
He et al. 2023 5.37 2.35 – 708 – – – –

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

Visualization

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