CWNU 428

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0.41 UTI
0.5
CN
0.3
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 10.0 [arcmin]
  • CN 0.5 Moderately populated
  • Cdens 0.3 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 428 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Relatively close Moderate extinction Near-solar metallicity Young

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 – 348.684 58.046 0.503 -3.678 -2.232 -43.484
Hunt & Reffert 2024 348.674 58.197 0.506 -3.67 -2.268 -40.107
Cavallo et al. 2024 348.721 58.072 0.505 – – –
Hunt & Reffert 2023 348.674 58.197 0.506 -3.67 -2.268 -40.107
He et al. 2022 348.729 58.161 0.52 -3.67 -2.22 –

💡 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 – – – – – 189* – –
Cavallo et al. 2024 2.11 1.91 – 69 0.500 – – –
Hunt & Reffert 2023 1.99 1.71 1.41 66 – – – –
He et al. 2022 1.86 1.80 – 100 0.370 – – –

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

Visualization

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