CWNU 498

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0.12 UTI
0.0
CN
0.08
Cdens
0.38
CC3
0.06
Clit
1.0
Cdup
Core radius and density 2.7 [pc], 0.4 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.08 Very loose
  • CC3 0.38 Low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 498 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, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is rarely studied 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)
Silver sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.06 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.06 (50th percentile).

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 344.861 61.079 0.428 -1.545 -1.0 –
Hunt & Reffert 2024 344.839 61.086 0.429 -1.555 -1.007 –
Cavallo et al. 2024 344.848 61.039 0.428 – – –
Hunt & Reffert 2023 344.839 61.086 0.429 -1.555 -1.007 –
He et al. 2022 344.812 61.055 0.42 -1.55 -1.01 –

💡 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– 2.185 3.33 2.41 78 -0.240 345 – –
Hunt & Reffert 2024 2.18 3.33 2.41 118 – 345(1) – –
Cavallo et al. 2024 2.19 3.20 – 38 0.100 – – –
Hunt & Reffert 2023 2.18 3.33 2.41 118 – – – –
He et al. 2022 4.27 4.63 – 2 -0.580 – – –

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

Visualization

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