CWNU 1677

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0.50 UTI
0.32
CN
0.92
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 4.6 [N/pc2]
  • CN 0.32 Poorly populated
  • Cdens 0.92 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1677 is a poorly populated, very dense object of high 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, intermediate-age cluster (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– 210.654 -59.414 0.343 -4.841 -2.881 -35.973
Hunt & Reffert 2024 210.687 -59.423 0.331 -4.851 -2.874 -35.844
Cavallo et al. 2024 210.533 -59.396 0.332 – – –
Hunt & Reffert 2023 210.687 -59.423 0.331 -4.851 -2.874 -35.844
He et al. 2023 210.615 -59.411 0.346 -4.83 -2.889 -36.39

💡 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– 2.63 2.84 2.17 355 0.280 445 – –
Hunt & Reffert 2024 – – – – – 445(1) – –
Cavallo et al. 2024 2.40 2.53 – 437 0.280 – – –
Hunt & Reffert 2023 2.70 2.84 2.17 159 – – – –
He et al. 2023 2.63 3.05 – 355 – – – –

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

Visualization

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