CWNU 260

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0.32 UTI
0.32
CN
0.29
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.4 [N/pc2]
  • CN 0.32 Poorly populated
  • Cdens 0.29 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 260 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a low-mass, metal-rich, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.

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

Palma et al. (2025)
Classified as genetic pair P197, along with CWNU_135.

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 117.471 -49.692 1.306 -4.712 7.787 16.724
Hunt & Reffert 2024 117.494 -49.718 1.263 -4.738 7.669 15.844
Cavallo et al. 2024 117.762 -49.712 1.276 – – –
Hunt & Reffert 2023 117.494 -49.718 1.263 -4.738 7.669 15.844
He et al. 2022 117.435 -49.658 1.3 -4.68 7.85 15.5

💡 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– 0.76 0.35 0.95 115 0.644 43 – –
Hunt & Reffert 2024 – – – – – 43(1) – –
Cavallo et al. 2024 0.76 0.35 – 166 0.320 – – –
Hunt & Reffert 2023 0.73 0.23 0.95 115 – – – –
He et al. 2022 0.91 0.48 – 79 0.968 – – –

(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 258 18.8 115.43 -50.08 1.38 -4.52 7.78 16.87 0.15

💡 Note: The % column shows the percentage of members that CWNU 260 shares with each listed object.

Visualization

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