CWNU 1680

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0.50 UTI
0.25
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 11.7 [N/pc2]
  • CN 0.25 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 1680 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 very high extinction. It is catalogued as a 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

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 301.213 29.447 0.279 -3.096 -4.856 15.804
Hunt & Reffert 2024 301.209 29.449 0.28 -3.117 -4.869 14.27
Cavallo et al. 2024 301.216 29.444 0.275 – – –
Hunt & Reffert 2023 301.209 29.449 0.28 -3.117 -4.869 14.27
He et al. 2023 301.217 29.457 0.292 -3.096 -4.854 15.8

💡 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– 3.21 5.09 2.31 86 0.230 481 – –
Hunt & Reffert 2024 – – – – – 481(1) – –
Cavallo et al. 2024 3.80 5.09 – 35 0.230 – – –
Hunt & Reffert 2023 3.21 5.17 2.31 86 – – – –
He et al. 2023 2.82 4.95 – 562 – – – –

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

Visualization

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