CWNU 2223

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0.65 UTI
0.75
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.2 [arcmin]
  • CN 0.75 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2223 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.
Distant High extinction Massive Near-solar metallicity Very young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 203.126 -62.288 0.237 -6.353 -1.243 -49.626
Hunt & Reffert 2024 203.119 -62.293 0.235 -6.367 -1.244 -49.645
Cavallo et al. 2024 203.105 -62.283 0.236 – – –
Hunt & Reffert 2023 203.119 -62.293 0.235 -6.367 -1.244 -49.645
He et al. 2023 203.116 -62.29 0.263 -6.333 -1.234 -45.53

💡 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 – – – – – 2566* – –
Cavallo et al. 2024 4.90 4.09 – 17 0.360 – – –
Hunt & Reffert 2023 4.14 4.31 2.85 32 – – – –
He et al. 2023 3.80 4.30 – 4 – – – –

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

Visualization

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