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
Radius (P>50% members) 100.0 [arcmin]
  • 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

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. 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.

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 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] Bfr BSS
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

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.

Visualization

Galactocentric position diagram

💡 Note: How are the galactocentric plots generated? See FAQ.