CWNU 1702

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0.45 UTI
0.0
CN
0.77
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 3.9 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.77 Dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1702 is a sparse, dense object of very 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 massive, near-solar metallicity, very young cluster (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– 258.416 -38.872 0.257 -1.061 -2.637 5.578
Hunt & Reffert 2024 258.397 -38.868 0.254 -1.058 -2.665 -53.16
Cavallo et al. 2024 258.428 -38.888 0.254 – – –
Hunt & Reffert 2023 258.397 -38.868 0.254 -1.058 -2.665 -53.16
He et al. 2023 258.43 -38.872 0.259 -1.038 -2.628 –

💡 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– 3.73 5.48 2.43 4 0.210 2618 – –
Hunt & Reffert 2024 – – – – – 2618(1) – –
Cavallo et al. 2024 3.73 5.33 – 4 0.210 – – –
Hunt & Reffert 2023 3.68 5.48 2.43 13 – – – –
He et al. 2023 4.47 6.80 – 4 – – – –

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

Visualization

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