CWNU 229

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0.56 UTI
0.54
CN
0.99
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 4.9 [N/pc2]
  • CN 0.54 Moderately populated
  • Cdens 0.99 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 229 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a metal-rich, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

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– 263.738 -43.035 0.917 -0.793 -1.736 19.238
Hunt & Reffert 2024 263.726 -43.016 0.898 -0.806 -1.797 14.734
Cavallo et al. 2024 263.726 -43.06 0.908 – – –
Hunt & Reffert 2023 263.726 -43.016 0.898 -0.806 -1.797 14.734
He et al. 2022 263.707 -43.049 0.92 -0.81 -1.74 –

💡 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– 1.07 0.55 0.57 105 0.681 236 – –
Hunt & Reffert 2024 – – – – – 236(1) – –
Cavallo et al. 2024 1.04 0.49 – 191 0.500 – – –
Hunt & Reffert 2023 1.07 0.55 0.57 105 – – – –
He et al. 2022 1.23 0.72 – 50 0.862 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14328 69.0 263.74 -43.02 0.92 -0.78 -1.72 19.91 0.0

💡 Note: The % column shows the percentage of members that CWNU 229 shares with each listed object.

Visualization

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