CWNU 2428

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0.38 UTI
0.37
CN
0.65
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.9 [arcmin]
  • CN 0.37 Poorly populated
  • Cdens 0.65 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2428 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close High extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 246.928 -51.152 0.336 -2.339 -3.77 -29.978
Hunt & Reffert 2024 246.925 -51.144 0.337 -2.226 -3.61 -22.494
Cavallo et al. 2024 246.904 -51.003 0.336 – – –
Hunt & Reffert 2023 246.925 -51.144 0.337 -2.226 -3.61 -22.494
He et al. 2023 246.964 -51.169 0.336 -2.374 -3.825 -16.71

💡 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
Hunt & Reffert 2024 – – – – – 298* – –
Cavallo et al. 2024 2.90 3.55 – 135 0.360 – – –
Hunt & Reffert 2023 2.74 3.65 2.83 35 – – – –
He et al. 2023 2.57 3.20 – 631 – – – –

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

Visualization

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