CWNU 1272

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0.31 UTI
0.3
CN
0.39
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.9 [N/pc2]
  • CN 0.3 Poorly populated
  • Cdens 0.39 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1272 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a moderate distance, above 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– 146.495 -51.898 0.385 -5.357 2.868 12.505
Hunt & Reffert 2024 146.507 -51.885 0.368 -5.399 2.877 –
Cavallo et al. 2024 146.451 -51.913 0.369 – – –
Hunt & Reffert 2023 146.507 -51.885 0.368 -5.399 2.877 –
He et al. 2023 146.525 -51.918 0.387 -5.349 2.852 12.51

💡 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– 2.46 2.11 1.12 141 0.560 114 – –
Hunt & Reffert 2024 – – – – – 114(1) – –
Cavallo et al. 2024 2.87 2.11 – 91 0.560 – – –
Hunt & Reffert 2023 2.46 1.76 1.12 252 – – – –
He et al. 2023 2.29 2.50 – 141 – – – –

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

Visualization

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