CWNU 1322

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0.47 UTI
0.37
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 6.8 [N/pc2]
  • CN 0.37 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 1322 is a poorly populated, very dense object of intermediate 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, young 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– 303.534 37.609 0.261 -3.823 -6.238 -18.227
Hunt & Reffert 2024 303.525 37.61 0.258 -3.824 -6.218 –
Cavallo et al. 2024 303.522 37.608 0.26 – – –
Hunt & Reffert 2023 303.525 37.61 0.258 -3.824 -6.218 –
He et al. 2023 303.529 37.616 0.273 -3.765 -6.248 -24.58

💡 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– 3.55 2.83 2.45 93 0.240 545 – –
Hunt & Reffert 2024 – – – – – 545(1) – –
Cavallo et al. 2024 3.55 2.60 – 102 0.240 – – –
Hunt & Reffert 2023 3.43 2.83 2.45 93 – – – –
He et al. 2023 4.47 3.50 – 5 – – – –

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

Visualization

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