CWNU 2333

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0.21 UTI
0.0
CN
0.2
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.2 Very loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 2333 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (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.

Distant Low extinction Near-solar metallicity Intermediate age

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 – 115.582 -25.897 0.235 -2.111 3.107 –
Hunt & Reffert 2024 115.561 -25.883 0.221 -2.103 3.072 76.66
Cavallo et al. 2024 115.543 -25.888 0.218 – – –
Hunt & Reffert 2023 115.561 -25.883 0.221 -2.103 3.072 76.66
He et al. 2023 115.557 -25.877 0.284 -2.11 3.17 76.54

💡 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 – – – – – 173* – –
Cavallo et al. 2024 3.94 1.49 – 32 -0.310 – – –
Hunt & Reffert 2023 3.64 0.89 1.24 206 – – – –
He et al. 2023 2.95 0.55 – 708 – – – –

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

Visualization

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