CWNU 1718

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0.16 UTI
0.25
CN
0.27
Cdens
0.12
CC3
0.3
Clit
0.64
Cdup
Stellar density (N50/rad) 1.4 [N/pc2]
  • CN 0.25 Poorly populated
  • Cdens 0.27 Loose
  • CC3 0.12 Very low quality
  • Clit 0.3 Poorly studied
  • Cdup 0.64 Likely unique

Overview

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CWNU 1718 is a poorly populated, loose object of very low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

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– 84.808 32.599 0.482 -0.257 -1.4 –
Zhang et al. 2024 84.805 32.609 – – – –
Hunt & Reffert 2024 84.805 32.609 0.478 -0.27 -1.392 –
Cavallo et al. 2024 84.827 32.542 0.475 – – –
Hunt & Reffert 2023 84.805 32.609 0.478 -0.27 -1.392 –
He et al. 2023 84.839 32.555 0.484 -0.28 -1.4 –

💡 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– 2.27 1.7 1.88 85 0.150 220 – –
Zhang et al. 2024 – – – – -0.099(1) – – –
Hunt & Reffert 2024 – – – – – 220(1) – –
Cavallo et al. 2024 2.27 1.70 – 85 0.400 – – –
Hunt & Reffert 2023 1.98 1.56 1.88 177 – – – –
He et al. 2023 2.29 1.70 – 11 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Teutsch J0538.2+3234 36.0 84.57 32.6 0.33 -0.22 -1.48 38.83 0.06

💡 Note: The % column shows the percentage of members that CWNU 1718 shares with each listed object.

Visualization

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