CWNU 534

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0.33 UTI
0.26
CN
0.39
Cdens
0.38
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 42.3 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 0.39 Loose
  • CC3 0.38 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 534 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Very close Low extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 273.367 26.495 3.383 -1.314 -5.589 -19.724
Wei et al. 2025 273.764 26.337 2.727 -1.696 -5.817 –
Cavallo et al. 2024 273.251 26.855 3.407 – – –
Hunt & Reffert 2023 273.257 27.475 3.404 -1.294 -5.636 -19.158
He et al. 2022 271.426 19.347 3.213 -1.202 -7.995 –
He et al. 2022 273.593 26.24 3.31 -1.23 -5.68 -20.3

💡 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] Bfr BSS
Wei et al. 2025 0.31 0.38 – 17 0.000 215 0.62 –
Cavallo et al. 2024 0.31 0.60 – 16 -0.020 – – –
Hunt & Reffert 2023 0.29 0.35 0.42 20 – – – –
He et al. 2022 – 0.60 – 35 – – – –
He et al. 2022 0.31 0.12 – 40 0.968 – – –

Visualization

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