CWNU 2124

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0.22 UTI
0.0
CN
0.22
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.22 Very loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 2124 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close High 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 – 64.926 53.988 0.291 0.686 -1.968 –
Hunt & Reffert 2024 64.909 54.054 0.3 0.688 -1.953 –
Cavallo et al. 2024 64.989 53.996 0.301 – – –
Hunt & Reffert 2023 64.909 54.054 0.3 0.688 -1.953 –
He et al. 2023 64.953 54.045 0.296 0.683 -1.948 –

💡 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 – – – – – 213* – –
Cavallo et al. 2024 2.98 3.26 – 123 0.080 – – –
Hunt & Reffert 2023 2.95 3.30 1.42 42 – – – –
He et al. 2023 2.82 3.60 – 8 – – – –

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

Visualization

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