CWNU 165

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0.43 UTI
0.0
CN
1.0
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 5.6 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 165 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, young cluster, but with a large variance across recent sources for the age and metallicity parameters (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– 290.088 4.326 0.686 0.112 -0.769 27.52
Hunt & Reffert 2024 290.082 4.33 0.679 0.047 -0.852 12.683
Cavallo et al. 2024 290.075 4.33 0.679 – – –
Hunt & Reffert 2023 290.082 4.33 0.679 0.047 -0.852 12.683
He et al. 2022 290.076 4.313 0.7 0.1 -0.77 –

💡 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– 1.61 1.76 1.03 69 -0.709 160 – –
Hunt & Reffert 2024 – – – – – 160(1) – –
Cavallo et al. 2024 1.61 2.32 – 69 0.610 – – –
Hunt & Reffert 2023 1.42 1.76 1.03 165 – – – –
He et al. 2022 2.04 1.26 – 3 -2.028 – – –

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

Visualization

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