CWNU 426

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0.42 UTI
0.34
CN
0.51
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 2.6 [N/pc2]
  • CN 0.34 Poorly populated
  • Cdens 0.51 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 426 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a metal-rich, 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– 208.693 -57.68 0.527 -3.509 -1.675 5.617
Hunt & Reffert 2024 208.692 -57.706 0.523 -3.507 -1.693 5.646
Cavallo et al. 2024 208.674 -57.68 0.529 – – –
Hunt & Reffert 2023 208.692 -57.706 0.523 -3.507 -1.693 5.646
He et al. 2022 208.677 -57.692 0.53 -3.52 -1.7 –

💡 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– 1.78 0.67 0.9 295 0.683 157 – –
Hunt & Reffert 2024 – – – – – 157(1) – –
Cavallo et al. 2024 1.79 0.83 – 295 0.450 – – –
Hunt & Reffert 2023 1.71 0.67 0.90 285 – – – –
He et al. 2022 1.78 0.48 – 398 0.916 – – –

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

Visualization

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