CWNU 2018

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0.22 UTI
0.0
CN
0.22
Cdens
0.75
CC3
0.06
Clit
1.0
Cdup
Core radius and density 1.4 [pc], 1.1 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.22 Very loose
  • CC3 0.75 High quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 2018 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the absorption and age parameters (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: 0.98 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.98 (50th percentile).

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 354.352 58.375 0.389 -0.007 -0.78 -44.48
Hunt & Reffert 2024 354.301 58.372 0.387 -0.058 -0.776 -43.378
Cavallo et al. 2024 354.328 58.409 0.389 – – –
Hunt & Reffert 2023 354.301 58.372 0.387 -0.058 -0.776 -43.378
He et al. 2023 354.371 58.375 0.393 -0.007 -0.792 –

💡 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– 2.415 2.09 0.86 152 0.290 106 – –
Hunt & Reffert 2024 2.43 2.09 0.86 152 – 106(1) – –
Cavallo et al. 2024 2.38 2.15 – 219 0.290 – – –
Hunt & Reffert 2023 2.43 2.09 0.86 152 – – – –
He et al. 2023 2.40 0.05 – 2 – – – –

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

Visualization

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