CWNU 1526

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0.31 UTI
0.43
CN
0.26
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.3 [N/pc2]
  • CN 0.43 Poorly populated
  • Cdens 0.26 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1526 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, 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– 103.46 -1.033 0.192 -0.426 0.709 61.96
Hunt & Reffert 2024 103.458 -1.03 0.173 -0.4 0.732 –
Cavallo et al. 2024 103.45 -1.038 0.169 – – –
Hunt & Reffert 2023 103.458 -1.03 0.173 -0.4 0.732 –
He et al. 2023 103.461 -1.03 0.289 -0.46 0.72 73.42

💡 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– 4.6 1.44 1.78 123 0.560 382 – –
Hunt & Reffert 2024 – – – – – 382(1) – –
Cavallo et al. 2024 4.45 1.21 – 79 0.560 – – –
Hunt & Reffert 2023 4.60 1.44 1.78 123 – – – –
He et al. 2023 4.68 1.65 – 158 – – – –

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

Visualization

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