CWNU 1331

Click to load Aladin Lite
0.39 UTI
0.25
CN
0.33
Cdens
0.75
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 1.6 [N/pc2]
  • CN 0.25 Poorly populated
  • Cdens 0.33 Loose
  • CC3 0.75 High quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1331 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Cavallo et al. (2024)
Gold sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 109.995 3.26 0.46 -1.989 -0.322 62.721
Hu & Soubiran 2025 110.003 3.241 – – – –
Hunt & Reffert 2024 109.983 3.206 0.468 -1.943 -0.35 62.715
Cavallo et al. 2024 110.003 3.242 0.47 – – –
Hunt & Reffert 2023 109.983 3.206 0.468 -1.943 -0.35 62.715
He et al. 2023 110.0 3.254 0.471 -1.975 -0.35 53.26

💡 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– 1.94 0.2 0.61 596 -0.120 131 – –
Hu & Soubiran 2025 – – – – -0.170(5) – – –
Hunt & Reffert 2024 – – – – – 131(1) – –
Cavallo et al. 2024 1.75 0.13 – 631 -0.070 – – –
Hunt & Reffert 2023 1.94 0.20 0.61 596 – – – –
He et al. 2023 2.09 0.60 – 251 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14085 76.0 109.99 3.23 0.45 -2.0 -0.31 62.72 0.03

💡 Note: The % column shows the percentage of members that CWNU 1331 shares with each listed object.

Visualization

â„šī¸