CWNU 1867

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0.29 UTI
0.29
CN
0.16
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 0.8 [N/pc2]
  • CN 0.29 Poorly populated
  • Cdens 0.16 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1867 is a poorly populated, very loose object of intermediate 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 (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– 138.649 -44.197 0.531 -3.112 1.435 –
Hunt & Reffert 2024 138.701 -44.248 0.52 -3.136 1.451 –
Cavallo et al. 2024 138.661 -44.223 0.526 – – –
Hunt & Reffert 2023 138.701 -44.248 0.52 -3.136 1.451 –
He et al. 2023 138.611 -44.188 0.529 -3.111 1.439 –

💡 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– 1.82 1.2 1.02 479 -0.060 85 – –
Hunt & Reffert 2024 – – – – – 85(1) – –
Cavallo et al. 2024 1.98 1.49 – 479 -0.060 – – –
Hunt & Reffert 2023 1.76 1.13 1.02 419 – – – –
He et al. 2023 1.82 1.20 – 708 – – – –

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

Visualization

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