CWNU 260

Click to load Aladin Lite
0.20 UTI
0.32
CN
0.07
Cdens
0.5
CC3
0.06
Clit
1.0
Cdup
Core radius and density 2.9 [pc], 0.4 [pc-2]
  • CN 0.32 Poorly populated
  • Cdens 0.07 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 260 is a poorly populated, very 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, near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely 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.

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.

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

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.96 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.96 (50th percentile).

Data

â„šī¸
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– 0.745 0.29 0.95 115 0.370 43 – –
Hunt & Reffert 2024 0.73 0.23 0.95 115 – 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 0.51 – 79 0.420 – – –

(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 0.14

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

Visualization

â„šī¸