CWNU 3593

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0.23 UTI
0.54
CN
0.01
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Core radius and density 18 [pc], 0.04 [pc-2]
  • CN 0.54 Moderately populated
  • Cdens 0.01 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 3593 is a moderately populated, very loose object of intermediate C3 quality. Its parallax locates it at a very large* distance, well below the mid-plane, affected by low extinction. It is catalogued as a very old cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~12.22 kpc) differs significantly from the median photometric distance (~6.46 kpc).

Note: This object contains blue stragglers according to at least one source.

Note: This object shares a very small percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

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.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 167.909 -67.891 0.082 -5.167 1.974 6.513
Cui et al. 2025 167.98 -67.883 0.1 -5.2 1.98 –
He et al. 2023 167.948 -67.89 0.095 -5.2 1.978 21.58

💡 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– 6.46 0.5 – 6310 – – – 2
Cui et al. 2025 – 0.40 – 6310 – – – 2(1)
He et al. 2023 6.46 0.60 – 6310 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4856 1.8 168.23 -67.75 0.23 -5.52 1.77 -21.62 0.03

💡 Note: The % column shows the percentage of members that CWNU 3593 shares with each listed object.

Visualization

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