CWNU 1760

Click to load Aladin Lite
0.12 UTI
0.0
CN
0.27
Cdens
0.12
CC3
0.1
Clit
1.0
Cdup
Core radius and density 1.1 [pc], 1.4 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.27 Loose
  • CC3 0.12 Very low quality
  • Clit 0.1 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1760 is a sparse, loose object of very low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported 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: 0.79 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.79 (50th percentile).

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 66.465 48.735 0.509 0.168 -2.391 90.298
Zhang et al. 2024 66.482 48.762 – – – –
Hunt & Reffert 2024 66.482 48.762 0.517 0.132 -2.359 115.844
Cavallo et al. 2024 66.478 48.725 0.516 – – –
Hunt & Reffert 2023 66.482 48.762 0.517 0.132 -2.359 115.844
He et al. 2023 66.465 48.743 0.518 0.168 -2.395 -28.06

💡 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– 1.945 3.76 2.275 196 0.060 154 – –
Zhang et al. 2024 – – – – 0.081(1) – – –
Hunt & Reffert 2024 1.85 3.55 2.28 196 – 154(1) – –
Cavallo et al. 2024 2.84 3.97 – 66 0.040 – – –
Hunt & Reffert 2023 1.85 3.55 2.27 196 – – – –
He et al. 2023 2.04 4.15 – 447 – – – –

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

Visualization

â„šī¸