CWNU 1707

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0.34 UTI
0.0
CN
0.46
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 2.3 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.46 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1707 is a sparse, loose object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age 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– 265.533 -37.297 0.664 0.159 -3.772 -8.652
Hunt & Reffert 2024 265.538 -37.373 0.644 0.187 -3.765 1.99
Cavallo et al. 2024 265.568 -37.333 0.655 – – –
Hunt & Reffert 2023 265.538 -37.373 0.644 0.187 -3.765 1.99
He et al. 2023 265.545 -37.326 0.667 0.159 -3.776 –

💡 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– 1.43 2.7 1.19 178 0.380 225 – –
Hunt & Reffert 2024 – – – – – 225(1) – –
Cavallo et al. 2024 1.43 2.84 – 178 0.380 – – –
Hunt & Reffert 2023 1.43 2.66 1.19 59 – – – –
He et al. 2023 1.41 2.70 – 251 – – – –

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

Visualization

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