CWNU 1893

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0.35 UTI
0.25
CN
0.77
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 3.8 [N/pc2]
  • CN 0.25 Poorly populated
  • Cdens 0.77 Dense
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1893 is a poorly populated, dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very 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– 289.532 10.7 0.433 0.916 -1.192 -11.053
Hunt & Reffert 2024 289.521 10.685 0.445 0.943 -1.245 -9.648
Cavallo et al. 2024 289.543 10.693 0.464 – – –
Hunt & Reffert 2023 289.521 10.685 0.445 0.943 -1.245 -9.648
He et al. 2023 289.541 10.683 0.435 0.917 -1.216 -11.05

💡 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– 2.04 5.08 2.23 355 0.110 610 – –
Hunt & Reffert 2024 – – – – – 610(1) – –
Cavallo et al. 2024 3.19 5.08 – 135 0.110 – – –
Hunt & Reffert 2023 2.03 5.01 2.23 380 – – – –
He et al. 2023 2.04 5.45 – 355 – – – –

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

Visualization

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