CWNU 2368

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0.51 UTI
0.31
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 10.7 [N/pc2]
  • CN 0.31 Poorly 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 2368 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above 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– 124.487 -33.46 0.205 -2.443 2.669 –
Hunt & Reffert 2024 124.488 -33.461 0.197 -2.454 2.698 –
Cavallo et al. 2024 124.487 -33.461 0.197 – – –
Hunt & Reffert 2023 124.488 -33.461 0.197 -2.454 2.698 –
He et al. 2023 124.492 -33.458 0.205 -2.464 2.678 –

💡 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– 4.07 1.25 1.78 398 -0.040 279 – –
Hunt & Reffert 2024 – – – – – 279(1) – –
Cavallo et al. 2024 3.73 1.32 – 427 -0.040 – – –
Hunt & Reffert 2023 5.34 1.03 1.78 211 – – – –
He et al. 2023 4.07 1.25 – 398 – – – –

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

Visualization

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