CWNU 2500

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0.36 UTI
0.26
CN
0.7
Cdens
0.25
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 3.5 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 0.7 Moderately dense
  • CC3 0.25 Low quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2500 is a poorly populated, moderately dense object of low 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 (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– 124.863 -37.543 0.234 -2.002 2.844 52.776
Hu & Soubiran 2025 124.886 -37.544 – – – –
Hunt & Reffert 2024 124.866 -37.533 0.257 -1.987 2.818 51.676
Cavallo et al. 2024 124.886 -37.544 0.247 – – –
Hunt & Reffert 2023 124.866 -37.533 0.257 -1.987 2.818 51.676
He et al. 2023 124.903 -37.527 0.253 -2.02 2.845 52.78

💡 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– 3.38 2.14 1.82 316 -0.005 359 – –
Hu & Soubiran 2025 – – – – -0.070(5) – – –
Hunt & Reffert 2024 – – – – – 359(1) – –
Cavallo et al. 2024 3.08 1.82 – 603 0.060 – – –
Hunt & Reffert 2023 3.38 2.14 1.82 265 – – – –
He et al. 2023 3.47 2.25 – 316 – – – –

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

Visualization

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