CWNU 230

Click to load Aladin Lite
0.43 UTI
0.36
CN
0.78
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 3.9 [N/pc2]
  • CN 0.36 Poorly populated
  • Cdens 0.78 Dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 230 is a poorly populated, dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, young 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)
Gold sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 270.121 -13.364 0.985 1.511 -0.805 -8.32
Hunt & Reffert 2024 270.135 -13.373 0.978 1.517 -0.786 -25.735
Cavallo et al. 2024 270.132 -13.355 0.982 – – –
Hunt & Reffert 2023 270.135 -13.373 0.978 1.517 -0.786 -25.735
He et al. 2022 270.123 -13.365 1.0 1.47 -0.77 –

💡 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– 1.02 1.9 1.37 79 0.618 166 – –
Hunt & Reffert 2024 – – – – – 166(1) – –
Cavallo et al. 2024 1.02 1.72 – 195 0.430 – – –
Hunt & Reffert 2023 0.95 1.90 1.37 76 – – – –
He et al. 2022 1.17 1.98 – 79 0.805 – – –

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

Visualization

â„šī¸