CWNU 189

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0.28 UTI
0.0
CN
0.64
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 3.2 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.64 Moderately dense
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 189 is a sparse, moderately dense object of low C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, 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– 95.04 -6.47 0.52 -1.359 2.034 –
Hunt & Reffert 2024 95.054 -6.442 0.523 -1.337 2.057 –
Cavallo et al. 2024 95.03 -6.442 0.516 – – –
Hunt & Reffert 2023 95.054 -6.442 0.523 -1.337 2.057 –
He et al. 2022 95.071 -6.493 0.55 -1.4 2.01 –

💡 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– 1.86 1.01 0.66 245 -0.532 117 – –
Hunt & Reffert 2024 – – – – – 117(1) – –
Cavallo et al. 2024 2.06 1.01 – 245 0.270 – – –
Hunt & Reffert 2023 1.86 0.95 0.66 199 – – – –
He et al. 2022 1.48 1.14 – 501 -1.335 – – –

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

Visualization

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