CWNU 2451

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0.40 UTI
0.53
CN
0.33
Cdens
0.5
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 6.1 [arcmin]
  • CN 0.53 Moderately populated
  • Cdens 0.33 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2451 is a moderately populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It was recently reported in the literature.
Relatively close Low extinction Near-solar metallicity Old

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 – 118.25 -25.226 0.305 -1.235 3.204 66.151
Hu & Soubiran 2025 118.234 -25.218 – – – –
Hunt & Reffert 2024 118.256 -25.206 0.316 -1.234 3.182 46.717
Cavallo et al. 2024 118.234 -25.219 0.311 – – –
Hunt & Reffert 2023 118.256 -25.206 0.316 -1.234 3.182 46.717
He et al. 2023 118.261 -25.238 0.309 -1.227 3.207 –

💡 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] Bfr BSS
Hu & Soubiran 2025 – – – – -0.190* – – –
Hunt & Reffert 2024 – – – – – 160* – –
Cavallo et al. 2024 2.45 0.46 – 1778 -0.300 – – –
Hunt & Reffert 2023 2.82 0.25 0.88 1426 – – – –
He et al. 2023 2.88 0.45 – 1259 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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