CWNU 19

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0.44 UTI
0.27
CN
0.67
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 3.3 [N/pc2]
  • CN 0.27 Poorly populated
  • Cdens 0.67 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 19 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, 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– 228.524 -54.529 0.49 -0.743 -1.714 –
Hunt & Reffert 2024 228.514 -54.536 0.494 -0.78 -1.758 1.434
Cavallo et al. 2024 228.455 -54.517 0.494 – – –
Hunt & Reffert 2023 228.514 -54.536 0.494 -0.78 -1.758 1.434
He et al. 2022 228.54 -54.522 0.46 -0.7 -1.74 –

💡 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– 1.85 1.65 1.5 63 0.543 275 – –
Hunt & Reffert 2024 – – – – – 275(1) – –
Cavallo et al. 2024 1.79 1.63 – 63 0.170 – – –
Hunt & Reffert 2023 1.85 1.65 1.50 77 – – – –
He et al. 2022 3.31 2.10 – 10 0.916 – – –

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

Visualization

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