CWNU 1780

Click to load Aladin Lite
0.40 UTI
0.0
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 6.9 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1780 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported 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– 5.709 62.238 0.467 -2.85 -1.628 –
Hunt & Reffert 2024 5.726 62.239 0.467 -2.856 -1.63 –
Cavallo et al. 2024 5.756 62.243 0.467 – – –
Hunt & Reffert 2023 5.726 62.239 0.467 -2.856 -1.63 –
He et al. 2023 5.722 62.239 0.466 -2.847 -1.629 –

💡 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– 2.04 1.21 0.77 8 0.020 237 – –
Hunt & Reffert 2024 – – – – – 237(1) – –
Cavallo et al. 2024 2.04 1.21 – 4 0.020 – – –
Hunt & Reffert 2023 1.99 1.03 0.77 8 – – – –
He et al. 2023 2.09 1.60 – 8 – – – –

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

Visualization

â„šī¸