CWNU 2325

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0.35 UTI
0.26
CN
0.25
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.2 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 0.25 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2325 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age 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– 291.038 -7.846 0.73 1.331 -2.156 -19.144
Hunt & Reffert 2024 291.041 -7.856 0.724 1.287 -2.18 -18.141
Cavallo et al. 2024 291.03 -7.845 0.728 – – –
Hunt & Reffert 2023 291.041 -7.856 0.724 1.287 -2.18 -18.141
He et al. 2023 291.032 -7.794 0.723 1.327 -2.182 -33.96

💡 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– 1.29 0.9 0.57 264 0.170 70 – –
Hunt & Reffert 2024 – – – – – 70(1) – –
Cavallo et al. 2024 1.45 1.28 – 245 0.170 – – –
Hunt & Reffert 2023 1.28 0.89 0.57 264 – – – –
He et al. 2023 1.29 0.90 – 891 – – – –

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

Visualization

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