CWNU 175

Click to load Aladin Lite
0.43 UTI
0.25
CN
1.0
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 7.2 [N/pc2]
  • CN 0.25 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 175 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.

Cavallo et al. (2024)
Silver sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 188.361 -63.512 0.704 -3.87 -1.18 5.45
Hunt & Reffert 2024 188.407 -63.515 0.689 -3.901 -1.186 1.411
Cavallo et al. 2024 188.176 -63.529 0.69 – – –
Hunt & Reffert 2023 188.407 -63.515 0.689 -3.901 -1.186 1.411
He et al. 2022 188.342 -63.53 0.7 -3.89 -1.19 7.5

💡 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– 1.12 1.8 2.51 126 0.149 187 – –
Hunt & Reffert 2024 – – – – – 187(1) – –
Cavallo et al. 2024 1.12 1.95 – 191 -0.670 – – –
Hunt & Reffert 2023 1.37 1.80 2.51 83 – – – –
He et al. 2022 1.10 1.62 – 126 0.968 – – –

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

Visualization

â„šī¸