CWNU 2407

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0.10 UTI
0.0
CN
0.1
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 14.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.1 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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CWNU 2407 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, 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 Moderate extinction Metal-rich Young

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 117.704 -32.737 0.62 -2.404 1.864 -11.473
Cavallo et al. 2024 117.672 -32.7 0.611 – – –
Hunt & Reffert 2023 117.696 -32.973 0.608 -2.404 1.848 -11.593
He et al. 2023 117.675 -32.769 0.621 -2.433 1.878 –

💡 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
Cavallo et al. 2024 1.71 1.20 – 58 0.520 – – –
Hunt & Reffert 2023 1.54 1.29 1.58 122 – – – –
He et al. 2023 1.55 1.75 – 35 – – – –

Visualization

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