CWNU 1939

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0.33 UTI
0.0
CN
0.42
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 2.1 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.42 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1939 is a sparse, loose object of high C3 quality. Its parallax locates it at a relatively close 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– 263.951 -35.677 0.76 1.218 -2.106 -3.64
Hunt & Reffert 2024 263.961 -35.68 0.75 1.205 -2.114 -3.6
Cavallo et al. 2024 263.99 -35.703 0.754 – – –
Hunt & Reffert 2023 263.961 -35.68 0.75 1.205 -2.114 -3.6
He et al. 2023 263.943 -35.679 0.764 1.208 -2.101 –

💡 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– 1.26 2.21 0.69 66 -0.060 137 – –
Hunt & Reffert 2024 – – – – – 137(1) – –
Cavallo et al. 2024 1.01 2.21 – 71 -0.060 – – –
Hunt & Reffert 2023 1.27 2.15 0.69 66 – – – –
He et al. 2023 1.26 2.50 – 25 – – – –

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

Visualization

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