CWNU 2439

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0.46 UTI
0.48
CN
0.93
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 4.6 [N/pc2]
  • CN 0.48 Poorly populated
  • Cdens 0.93 Very dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2439 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, near 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– 253.712 -43.858 0.606 -1.896 -2.536 –
Hunt & Reffert 2024 253.712 -43.864 0.607 -1.865 -2.529 –
Cavallo et al. 2024 253.708 -43.859 0.609 – – –
Hunt & Reffert 2023 253.712 -43.864 0.607 -1.865 -2.529 –
He et al. 2023 253.725 -43.867 0.61 -1.891 -2.532 –

💡 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– 1.51 2.71 1.4 39 0.120 301 – –
Hunt & Reffert 2024 – – – – – 301(1) – –
Cavallo et al. 2024 1.39 2.66 – 324 0.120 – – –
Hunt & Reffert 2023 1.57 2.71 1.40 39 – – – –
He et al. 2023 1.51 3.10 – 22 – – – –

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

Visualization

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