CWNU 1442

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0.55 UTI
0.51
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 8.7 [N/pc2]
  • CN 0.51 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1442 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above 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– 201.699 -60.919 0.286 -5.622 -1.59 -39.23
Hunt & Reffert 2024 201.677 -60.92 0.293 -5.634 -1.592 -39.386
Cavallo et al. 2024 201.689 -60.912 0.291 – – –
Hunt & Reffert 2023 201.677 -60.92 0.293 -5.634 -1.592 -39.386
He et al. 2023 201.661 -60.917 0.287 -5.62 -1.591 -28.18

💡 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– 2.97 3.14 2.24 221 0.020 951 – –
Hunt & Reffert 2024 – – – – – 951(1) – –
Cavallo et al. 2024 2.69 3.14 – 331 0.020 – – –
Hunt & Reffert 2023 2.97 3.01 2.24 221 – – – –
He et al. 2023 3.09 3.65 – 141 – – – –

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

Visualization

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