CWNU 4128

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0.25 UTI
0.32
CN
0.18
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.9 [N/pc2]
  • CN 0.32 Poorly populated
  • Cdens 0.18 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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CWNU 4128 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 young cluster (see Parameters). It was recently reported in the literature.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 120.755 -31.479 0.293 -2.632 2.814 –
He et al. 2023 120.76 -31.494 0.293 -2.632 2.814 –

💡 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– 3.16 1.1 – 63 – – – –
He et al. 2023 3.16 1.10 – 63 – – – –

Visualization

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