CWNU 1435

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0.39 UTI
0.26
CN
0.46
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 2.3 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 0.46 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1435 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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– 229.893 -57.678 0.65 -4.377 -4.595 0.815
Hunt & Reffert 2024 229.844 -57.734 0.66 -4.395 -4.59 -0.4
Cavallo et al. 2024 229.854 -57.666 0.658 – – –
Hunt & Reffert 2023 229.844 -57.734 0.66 -4.395 -4.59 -0.4
He et al. 2023 229.89 -57.628 0.656 -4.375 -4.583 0.82

💡 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– 1.45 3.05 1.2 331 -0.270 232 – –
Hunt & Reffert 2024 – – – – – 232(1) – –
Cavallo et al. 2024 1.10 3.13 – 331 -0.270 – – –
Hunt & Reffert 2023 1.49 3.02 1.20 203 – – – –
He et al. 2023 1.45 3.05 – 398 – – – –

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

Visualization

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