CWNU 162

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0.25 UTI
0.27
CN
0.24
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.2 [N/pc2]
  • CN 0.27 Poorly populated
  • Cdens 0.24 Very loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 162 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, above 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 is poorly studied in the literature.

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– 327.808 58.132 0.765 -2.319 -3.729 -14.911
Hunt & Reffert 2024 327.813 58.119 0.762 -2.331 -3.695 -28.299
Cavallo et al. 2024 327.859 58.234 0.764 – – –
Hunt & Reffert 2023 327.813 58.119 0.762 -2.331 -3.695 -28.299
He et al. 2022 327.696 58.105 0.79 -2.3 -3.7 –

💡 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– 1.25 2.22 1.25 101 0.073 94 – –
Hunt & Reffert 2024 – – – – – 94(1) – –
Cavallo et al. 2024 1.16 2.43 – 191 -0.310 – – –
Hunt & Reffert 2023 1.25 2.22 1.25 101 – – – –
He et al. 2022 1.32 2.10 – 50 0.457 – – –

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

Visualization

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