CWNU 1920

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0.56 UTI
0.3
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 5.2 [N/pc2]
  • CN 0.3 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 1920 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, 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)
Wood sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 260.104 -40.654 0.377 -0.503 -1.116 -2.857
Hunt & Reffert 2024 260.102 -40.659 0.375 -0.473 -1.102 9.135
Cavallo et al. 2024 260.085 -40.661 0.38 – – –
Hunt & Reffert 2023 260.102 -40.659 0.375 -0.473 -1.102 9.135
He et al. 2023 260.077 -40.649 0.388 -0.468 -1.126 –

💡 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– 3.02 4.68 3.12 22 0.560 1066 – –
Hunt & Reffert 2024 – – – – – 1066(1) – –
Cavallo et al. 2024 3.22 4.37 – 22 0.560 – – –
Hunt & Reffert 2023 2.39 4.68 3.12 37 – – – –
He et al. 2023 3.02 5.95 – 2 – – – –

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

Visualization

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