CWNU 2180

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0.21 UTI
0.0
CN
0.24
Cdens
0.12
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad) 1.2 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.24 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.35 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2180 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a relatively close distance, near 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 metallicity parameter (see Parameters). It was recently reported in the literature.

Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 112 along with HSC_1387.

Palma et al. (2025)
Classified as optical pair P343, along with HSC_1387.

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 99999– 83.138 30.578 0.775 -1.262 -4.217 -21.013
Zhang et al. 2024 83.15 30.602 – – – –
Hunt & Reffert 2024 83.15 30.602 0.773 -1.22 -4.235 -20.94
Cavallo et al. 2024 83.078 30.655 0.773 – – –
Hunt & Reffert 2023 83.15 30.602 0.773 -1.22 -4.235 -20.94
He et al. 2023 83.117 30.565 0.777 -1.264 -4.225 –

💡 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– 1.335 1.795 0.64 212 -0.080 72 – –
Liu et al. 2025 3.10 0.67 – 200 – – – –
Zhang et al. 2024 – – – – -0.399(1) – – –
Hunt & Reffert 2024 – – – – – 72(1) – –
Cavallo et al. 2024 1.32 1.89 – 224 0.240 – – –
Hunt & Reffert 2023 1.26 1.70 0.64 136 – – – –
He et al. 2023 1.35 2.00 – 251 – – – –

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

Visualization

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