CWNU 2422

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0.42 UTI
0.54
CN
0.71
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.4 [arcmin]
  • CN 0.54 Moderately populated
  • Cdens 0.71 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2422 is a moderately populated, moderately dense object of low C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Very distant 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 – 130.886 -47.612 0.174 -2.774 3.687 –
Hunt & Reffert 2024 130.873 -47.603 0.172 -2.776 3.684 –
Cavallo et al. 2024 130.895 -47.609 0.173 – – –
Hunt & Reffert 2023 130.873 -47.603 0.172 -2.776 3.684 –
He et al. 2023 130.871 -47.591 0.196 -2.781 3.671 –

💡 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 – – – – – 697* – –
Cavallo et al. 2024 3.31 2.38 – 79 -0.360 – – –
Hunt & Reffert 2023 5.54 2.45 1.98 23 – – – –
He et al. 2023 6.61 2.95 – 4 – – – –

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

Visualization

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