CWNU 1434

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0.52 UTI
0.33
CN
1.0
Cdens
0.75
CC3
0.3
Clit
0.97
Cdup
Stellar density (N50/rad) 18.1 [N/pc2]
  • CN 0.33 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.3 Poorly studied
  • Cdup 0.97 Unique

Overview

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CWNU 1434 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This is a unique object, which shares a very small percentage of members with at least one previously 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– 117.133 -25.766 0.215 -2.54 3.221 –
Hu & Soubiran 2025 117.128 -25.763 – – – –
Hunt & Reffert 2024 117.136 -25.772 0.214 -2.552 3.228 126.511
Cavallo et al. 2024 117.128 -25.763 0.212 – – –
Hunt & Reffert 2023 117.136 -25.772 0.214 -2.552 3.228 126.511
He et al. 2023 117.132 -25.769 0.222 -2.543 3.198 –

💡 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– 4.79 1.15 0.68 891 -0.260 218 – –
Hu & Soubiran 2025 – – – – -0.210(5) – – –
Hunt & Reffert 2024 – – – – – 218(1) – –
Cavallo et al. 2024 4.27 1.16 – 891 -0.310 – – –
Hunt & Reffert 2023 4.91 0.64 0.68 1119 – – – –
He et al. 2023 4.79 1.15 – 794 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Haffner 25 3.0 117.15 -25.95 0.24 -2.64 3.5 – 0.16

💡 Note: The % column shows the percentage of members that CWNU 1434 shares with each listed object.

Visualization

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