CWNU 58

Click to load Aladin Lite
0.49 UTI
0.69
CN
0.62
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 3.1 [N/pc2]
  • CN 0.69 Moderately populated
  • Cdens 0.62 Moderately dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 58 is a moderately populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is poorly studied in the literature.

Palma et al. (2025)
Part of multiple system G261, along with OC_0192 and Theia_1001.

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– 342.006 60.669 1.14 -0.282 -2.44 -14.226
Hunt & Reffert 2024 342.159 60.541 1.134 -0.21 -2.4 -27.477
Cavallo et al. 2024 341.908 60.701 1.142 – – –
Hunt & Reffert 2023 342.159 60.541 1.134 -0.21 -2.4 -27.477
He et al. 2022 341.899 60.908 1.15 -0.5 -2.49 –

💡 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– 0.91 3.11 1.69 8 -0.260 160 – –
Hunt & Reffert 2024 – – – – – 160(1) – –
Cavallo et al. 2024 0.91 3.19 – 14 -0.100 – – –
Hunt & Reffert 2023 0.85 3.11 1.69 8 – – – –
He et al. 2022 1.07 1.02 – 1 -0.419 – – –

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

Visualization

â„šī¸