CWNU 1143

(OCSN 182)

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0.60 UTI
0.52
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 5.4 [N/pc2]
  • CN 0.52 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1143 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It is poorly studied in the literature.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 239.229 -25.305 9.293 -21.947 -33.402 -3.2
Cavallo et al. 2024 239.858 -25.188 9.23 – – –
Hunt & Reffert 2023 239.071 -25.701 9.244 -21.492 -33.359 -1.914
Qin et al. 2023 239.37 -25.73 9.19 -20.55 -32.66 -4.36
He et al. 2022 239.637 -25.254 9.332 -21.962 -33.816 –

💡 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– 0.11 0.29 0.54 25 0.170 – – –
Cavallo et al. 2024 0.11 1.10 – 48 0.170 – – –
Hunt & Reffert 2023 0.11 0.36 0.54 18 – – – –
Qin et al. 2023 0.11 0.22 – 25 – – – –
He et al. 2022 – 0.05 – 25 – – – –

Visualization

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