CWNU 2390

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0.18 UTI
0.32
CN
0.07
Cdens
0.38
CC3
0.06
Clit
1.0
Cdup
Core radius and density 2.2 [pc], 0.3 [pc-2]
  • CN 0.32 Poorly populated
  • Cdens 0.07 Very loose
  • CC3 0.38 Low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 2390 is a poorly populated, 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, 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.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.18 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.18 (50th percentile).

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 327.414 54.826 0.287 -4.239 -4.053 –
Hunt & Reffert 2024 327.414 54.831 0.282 -4.205 -4.058 –
Cavallo et al. 2024 327.418 54.828 0.288 – – –
Hunt & Reffert 2023 327.414 54.831 0.282 -4.205 -4.058 –
He et al. 2023 327.408 54.815 0.319 -4.244 -4.045 -50.58

💡 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] Bfrac BSS
UCC 99999– 2.92 3.23 2.41 76 -0.440 251 – –
Hunt & Reffert 2024 3.15 3.23 2.41 76 – 251(1) – –
Cavallo et al. 2024 2.69 3.80 – 29 -0.440 – – –
Hunt & Reffert 2023 3.15 3.23 2.41 76 – – – –
He et al. 2023 2.69 2.95 – 447 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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