CWNU 164

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0.34 UTI
0.38
CN
0.55
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 2.8 [N/pc2]
  • CN 0.38 Poorly populated
  • Cdens 0.55 Moderately dense
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 164 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, 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– 136.766 -44.285 0.924 -9.504 7.718 12.831
Hunt & Reffert 2024 136.794 -44.31 0.91 -9.527 7.7 -7.272
Cavallo et al. 2024 136.747 -44.277 0.929 – – –
Hunt & Reffert 2023 136.794 -44.31 0.91 -9.527 7.7 -7.272
He et al. 2022 136.814 -44.267 0.93 -9.51 7.71 –

💡 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– 1.04 1.17 0.65 199 -0.211 97 – –
Hunt & Reffert 2024 – – – – – 97(1) – –
Cavallo et al. 2024 1.07 1.17 – 214 0.220 – – –
Hunt & Reffert 2023 1.04 0.88 0.65 199 – – – –
He et al. 2022 0.87 1.20 – 63 -0.642 – – –

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

Visualization

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