CWNU 1342

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0.55 UTI
0.5
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 8.9 [N/pc2]
  • CN 0.5 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 1342 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (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– 200.272 -63.194 0.279 -6.586 -1.361 -25.431
Hunt & Reffert 2024 200.281 -63.197 0.279 -6.58 -1.358 -25.431
Cavallo et al. 2024 200.294 -63.187 0.279 – – –
Hunt & Reffert 2023 200.281 -63.197 0.279 -6.58 -1.358 -25.431
He et al. 2023 200.277 -63.2 0.28 -6.58 -1.363 -25.43

💡 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– 3.24 2.41 1.46 141 -0.040 628 – –
Hunt & Reffert 2024 – – – – – 628(1) – –
Cavallo et al. 2024 2.26 2.08 – 316 -0.040 – – –
Hunt & Reffert 2023 3.31 2.41 1.46 87 – – – –
He et al. 2023 3.24 2.45 – 141 – – – –

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

Visualization

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