CWNU 1459

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0.63 UTI
0.56
CN
1.0
Cdens
1.0
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 6.9 [N/pc2]
  • CN 0.56 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1459 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, well above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the absorption and age parameters (see Parameters). It was recently reported in the literature.

Note: This object shares a large 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– 145.59 -38.461 0.242 -5.673 4.28 30.489
Hu & Soubiran 2025 145.6 -38.463 – – – –
Hunt & Reffert 2024 145.585 -38.458 0.234 -5.674 4.285 30.44
Cavallo et al. 2024 145.6 -38.463 0.236 – – –
Hunt & Reffert 2023 145.585 -38.458 0.234 -5.674 4.285 30.44
He et al. 2023 145.591 -38.455 0.243 -5.681 4.269 30.49

💡 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– 3.76 0.67 0.25 2742 -0.280 394 – –
Hu & Soubiran 2025 – – – – -0.190(5) – – –
Hunt & Reffert 2024 – – – – – 394(1) – –
Cavallo et al. 2024 2.73 0.67 – 5012 -0.370 – – –
Hunt & Reffert 2023 3.76 0.30 0.25 2742 – – – –
He et al. 2023 5.13 1.90 – 316 – – – –

(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 3225 77.4 145.59 -38.46 0.24 -5.68 4.29 30.49 0.02

💡 Note: The % column shows the percentage of members that CWNU 1459 shares with each listed object.

Visualization

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