CWNU 1340

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0.38 UTI
0.0
CN
0.67
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 3.3 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.67 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1340 is a sparse, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, above 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– 235.177 -51.792 0.587 -2.377 -2.257 -31.489
Hunt & Reffert 2024 235.204 -51.817 0.594 -2.355 -2.24 -40.004
Cavallo et al. 2024 235.192 -51.796 0.595 – – –
Hunt & Reffert 2023 235.204 -51.817 0.594 -2.355 -2.24 -40.004
He et al. 2023 235.203 -51.799 0.603 -2.387 -2.24 –

💡 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– 1.56 1.2 0.55 45 0.100 124 – –
Hunt & Reffert 2024 – – – – – 124(1) – –
Cavallo et al. 2024 1.72 1.64 – 43 0.100 – – –
Hunt & Reffert 2023 1.56 0.98 0.55 132 – – – –
He et al. 2023 1.55 1.20 – 45 – – – –

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

Visualization

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