CWNU 1813

Click to load Aladin Lite
0.56 UTI
0.29
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 14.6 [N/pc2]
  • CN 0.29 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1813 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported 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– 295.235 22.62 0.227 -2.208 -4.326 12.638
Hunt & Reffert 2024 295.233 22.625 0.22 -2.202 -4.339 36.573
Cavallo et al. 2024 295.22 22.625 0.223 – – –
Hunt & Reffert 2023 295.233 22.625 0.22 -2.202 -4.339 36.573
He et al. 2023 295.227 22.618 0.234 -2.213 -4.323 12.03

💡 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– 3.79 5.48 2.4 89 0.230 1647 – –
Hunt & Reffert 2024 – – – – – 1647(1) – –
Cavallo et al. 2024 4.19 5.39 – 60 0.230 – – –
Hunt & Reffert 2023 3.79 5.48 2.40 362 – – – –
He et al. 2023 3.63 6.30 – 89 – – – –

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

Visualization

â„šī¸