CWNU 1421

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0.49 UTI
0.47
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 6.7 [N/pc2]
  • CN 0.47 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1421 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below 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.

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– 77.822 34.199 0.33 -0.883 -1.109 -7.832
Hunt & Reffert 2024 77.819 34.191 0.328 -0.868 -1.098 -7.69
Cavallo et al. 2024 77.81 34.215 0.324 – – –
Hunt & Reffert 2023 77.819 34.191 0.328 -0.868 -1.098 -7.69
He et al. 2023 77.821 34.204 0.313 -0.879 -1.108 -7.83

💡 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– 2.63 1.8 1.3 324 -0.070 200 – –
Hunt & Reffert 2024 – – – – – 200(1) – –
Cavallo et al. 2024 2.47 1.76 – 324 -0.070 – – –
Hunt & Reffert 2023 2.76 1.92 1.30 178 – – – –
He et al. 2023 2.63 1.80 – 562 – – – –

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

Visualization

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