CWNU 23

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0.33 UTI
0.0
CN
0.42
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.42 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 23 is a sparse, loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, young cluster (see Parameters). It is poorly studied in the literature.
Distant High extinction Massive Metal-rich 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 – 342.923 61.654 0.275 -2.878 -1.578 -73.685
Hunt & Reffert 2024 342.929 61.643 0.275 -2.896 -1.608 -55.017
Cavallo et al. 2024 342.9 61.517 0.274 – – –
Hunt & Reffert 2023 342.929 61.643 0.275 -2.896 -1.608 -55.017
He et al. 2022 342.912 61.65 0.26 -2.89 -1.58 -64.6

💡 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 – – – – – 1297* – –
Cavallo et al. 2024 3.89 3.49 – 25 0.720 – – –
Hunt & Reffert 2023 3.30 3.77 2.51 20 – – – –
He et al. 2022 3.47 4.20 – 6 0.968 – – –

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

Visualization

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