CWNU 1807

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0.31 UTI
0.0
CN
0.8
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 4.0 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.8 Dense
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1807 is a sparse, dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, 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– 77.236 40.501 0.368 0.163 -0.821 -18.564
Hunt & Reffert 2024 77.279 40.505 0.371 0.144 -0.809 -28.88
Cavallo et al. 2024 77.248 40.536 0.366 – – –
Hunt & Reffert 2023 77.279 40.505 0.371 0.144 -0.809 -28.88
He et al. 2023 77.244 40.513 0.378 0.172 -0.826 -23.82

💡 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– 2.54 1.15 1.2 490 0.650 145 – –
Hunt & Reffert 2024 – – – – – 145(1) – –
Cavallo et al. 2024 2.54 0.99 – 490 0.650 – – –
Hunt & Reffert 2023 2.55 1.15 1.20 417 – – – –
He et al. 2023 2.40 1.40 – 631 – – – –

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

Visualization

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