CWNU 1431

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0.25 UTI
0.0
CN
0.23
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.2 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.23 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1431 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age 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– 107.91 -14.937 0.397 -1.49 1.407 –
Hunt & Reffert 2024 107.971 -14.927 0.387 -1.494 1.348 –
Cavallo et al. 2024 107.918 -14.941 0.392 – – –
Hunt & Reffert 2023 107.971 -14.927 0.387 -1.494 1.348 –
He et al. 2023 107.909 -14.965 0.389 -1.511 1.386 –

💡 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– 2.31 1.03 0.92 355 -0.270 221 – –
Hunt & Reffert 2024 – – – – – 221(1) – –
Cavallo et al. 2024 2.25 1.03 – 275 -0.270 – – –
Hunt & Reffert 2023 2.31 0.85 0.92 405 – – – –
He et al. 2023 2.34 1.20 – 355 – – – –

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

Visualization

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