CWNU 1540

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0.35 UTI
0.34
CN
0.14
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 0.7 [N/pc2]
  • CN 0.34 Poorly populated
  • Cdens 0.14 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1540 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young 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– 109.874 -15.892 0.311 -2.642 2.962 –
Hunt & Reffert 2024 109.904 -15.936 0.311 -2.646 2.948 76.473
Cavallo et al. 2024 109.818 -15.772 0.313 – – –
Hunt & Reffert 2023 109.904 -15.936 0.311 -2.646 2.948 76.473
He et al. 2023 109.817 -15.785 0.313 -2.616 2.935 –

💡 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– 2.83 1.25 1.27 76 -0.170 216 – –
Hunt & Reffert 2024 – – – – – 216(1) – –
Cavallo et al. 2024 2.74 1.35 – 76 -0.170 – – –
Hunt & Reffert 2023 2.83 1.15 1.27 77 – – – –
He et al. 2023 2.95 1.25 – 40 – – – –

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

Visualization

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