CWNU 111

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0.28 UTI
0.0
CN
0.53
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 2.6 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.53 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 111 is a sparse, moderately dense object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by high 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– 28.35 67.807 0.611 -2.205 0.603 -13.261
Hunt & Reffert 2024 28.686 67.813 0.638 -2.217 0.625 -8.696
Cavallo et al. 2024 28.583 67.815 0.638 – – –
Hunt & Reffert 2023 28.686 67.813 0.638 -2.217 0.625 -8.696
He et al. 2022 28.246 67.798 0.63 -2.22 0.61 -33.2

💡 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– 1.49 3.62 1.59 77 0.698 138 – –
Hunt & Reffert 2024 – – – – – 138(1) – –
Cavallo et al. 2024 1.90 3.62 – 23 0.480 – – –
Hunt & Reffert 2023 1.49 3.92 1.59 77 – – – –
He et al. 2022 1.20 3.18 – 501 0.916 – – –

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

Visualization

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