CWNU 1643

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0.50 UTI
0.27
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 16.2 [N/pc2]
  • CN 0.27 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1643 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very 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)
Gold 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– 199.039 -63.422 0.203 -6.841 -0.97 -25.556
Hunt & Reffert 2024 199.05 -63.426 0.198 -6.85 -0.967 -6.063
Cavallo et al. 2024 199.041 -63.418 0.198 – – –
Hunt & Reffert 2023 199.05 -63.426 0.198 -6.85 -0.967 -6.063
He et al. 2023 199.051 -63.421 0.205 -6.851 -0.984 –

💡 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– 4.65 3.73 2.19 7 0.240 505 – –
Hunt & Reffert 2024 – – – – – 505(1) – –
Cavallo et al. 2024 3.65 3.25 – 138 0.240 – – –
Hunt & Reffert 2023 4.65 3.73 2.19 7 – – – –
He et al. 2023 5.25 4.30 – 5 – – – –

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

Visualization

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