CWNU 1425

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0.50 UTI
0.51
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 6.6 [N/pc2]
  • CN 0.51 Moderately 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 1425 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-poor, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Cavallo et al. (2024)
Silver 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– 279.686 -6.948 0.549 0.455 -4.889 15.207
Hunt & Reffert 2024 279.722 -6.909 0.541 0.467 -4.911 33.378
Cavallo et al. 2024 279.676 -6.986 0.548 – – –
Hunt & Reffert 2023 279.722 -6.909 0.541 0.467 -4.911 33.378
He et al. 2023 279.682 -6.948 0.559 0.459 -4.903 14.51

💡 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– 1.62 3.45 2.61 353 -0.800 828 – –
Hunt & Reffert 2024 – – – – – 828(1) – –
Cavallo et al. 2024 1.47 4.29 – 257 -0.800 – – –
Hunt & Reffert 2023 1.70 3.40 2.61 353 – – – –
He et al. 2023 1.62 3.45 – 708 – – – –

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

Visualization

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