CWNU 1832

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0.41 UTI
0.29
CN
0.75
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 3.8 [N/pc2]
  • CN 0.29 Poorly populated
  • Cdens 0.75 Dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1832 is a poorly populated, dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported 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– 257.689 -36.028 0.567 1.348 0.441 -29.438
Hunt & Reffert 2024 257.692 -36.029 0.561 1.334 0.408 -29.454
Cavallo et al. 2024 257.683 -36.023 0.569 – – –
Hunt & Reffert 2023 257.692 -36.029 0.561 1.334 0.408 -29.454
He et al. 2023 257.695 -36.015 0.581 1.366 0.443 -29.44

💡 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– 1.65 3.65 2.17 123 -0.330 400 – –
Hunt & Reffert 2024 – – – – – 400(1) – –
Cavallo et al. 2024 1.58 3.65 – 123 -0.330 – – –
Hunt & Reffert 2023 1.65 3.44 2.17 96 – – – –
He et al. 2023 1.66 3.65 – 141 – – – –

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

Visualization

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