CWNU 2498

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0.28 UTI
0.27
CN
0.17
Cdens
0.38
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 0.9 [N/pc2]
  • CN 0.27 Poorly populated
  • Cdens 0.17 Very loose
  • CC3 0.38 Low quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2498 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, old 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– 194.788 -60.686 0.337 -8.56 -1.8 -6.42
Hu & Soubiran 2025 194.775 -60.676 – – – –
Hunt & Reffert 2024 194.774 -60.681 0.331 -8.549 -1.808 -6.758
Cavallo et al. 2024 194.775 -60.676 0.332 – – –
Hunt & Reffert 2023 194.774 -60.681 0.331 -8.549 -1.808 -6.758
He et al. 2023 194.787 -60.687 0.342 -8.549 -1.775 -6.42

💡 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– 2.77 1.55 0.86 1000 -0.590 157 – –
Hunt & Reffert 2024 – – – – – 157(1) – –
Cavallo et al. 2024 2.77 2.02 – 1096 -0.590 – – –
Hunt & Reffert 2023 2.99 1.55 0.86 867 – – – –
He et al. 2023 2.69 1.55 – 1000 – – – –

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

Visualization

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