CWNU 1819

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0.33 UTI
0.0
CN
0.76
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 3.8 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.76 Dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1819 is a sparse, dense object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

Cavallo et al. (2024)
Bronze 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– 352.762 67.357 0.482 -3.002 -0.856 -27.906
Hunt & Reffert 2024 352.742 67.357 0.481 -2.965 -0.842 -22.3
Cavallo et al. 2024 352.727 67.381 0.478 – – –
Hunt & Reffert 2023 352.742 67.357 0.481 -2.965 -0.842 -22.3
He et al. 2023 352.717 67.365 0.488 -2.979 -0.858 -27.91

💡 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– 1.99 4.85 1.85 420 -0.120 330 – –
Hunt & Reffert 2024 – – – – – 330(1) – –
Cavallo et al. 2024 2.41 4.85 – 234 -0.120 – – –
Hunt & Reffert 2023 1.99 5.14 1.85 420 – – – –
He et al. 2023 1.86 4.50 – 1000 – – – –

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

Visualization

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