CWNU 1029

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0.45 UTI
0.54
CN
0.58
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 2.9 [N/pc2]
  • CN 0.54 Moderately populated
  • Cdens 0.58 Moderately dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1029 is a moderately populated, moderately dense object of intermediate 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, very young cluster (see Parameters). It is poorly studied 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– 49.0 59.725 0.903 0.596 -1.722 -11.817
Hunt & Reffert 2024 48.933 59.643 0.912 0.618 -1.675 -10.682
Cavallo et al. 2024 49.079 59.713 0.913 – – –
Hunt & Reffert 2023 48.933 59.643 0.912 0.618 -1.675 -10.682
He et al. 2022 49.131 59.73 0.909 0.558 -1.575 –

💡 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– 1.135 2.49 1.02 7 -0.140 64 – –
Hunt & Reffert 2024 – – – – – 64(1) – –
Cavallo et al. 2024 1.22 2.49 – 7 -0.140 – – –
Hunt & Reffert 2023 1.05 2.47 1.02 5 – – – –
He et al. 2022 – 3.00 – 14 – – – –

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

Visualization

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