CWNU 3267

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0.04 UTI
0.61
CN
0.53
Cdens
0.75
CC3
0.0
Clit
0.11
Cdup
Core radius and density 1.7 [pc], 2.6 [pc-2]
  • CN 0.61 Moderately populated
  • Cdens 0.53 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.11 Likely duplicate

Overview

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CWNU 3267 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

(*): The parallax distance estimate (~7.02 kpc) differs significantly from the median photometric distance (~4.90 kpc).

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 200.909 -63.67 0.142 -6.348 -1.01 -11.987
Cui et al. 2025 200.909 -63.673 0.14 -6.34 -1.02 –
He et al. 2023 200.907 -63.669 0.142 -6.344 -1.024 -11.99

💡 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– 4.9 2.705 – 1190 – – – 17
Cui et al. 2025 – 2.71 – 794 – – – 17(1)
He et al. 2023 4.90 2.70 – 1585 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Teutsch 79 88.9 200.91 -63.67 0.14 -6.35 -1.01 -11.99 0.51

💡 Note: The % column shows the percentage of members that CWNU 3267 shares with each listed object.

Visualization

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