CWNU 1909

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0.42 UTI
0.26
CN
0.82
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 4.1 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 0.82 Dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1909 is a poorly populated, dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (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– 24.915 57.488 0.555 -0.981 -1.696 –
Hunt & Reffert 2024 24.889 57.449 0.538 -0.961 -1.682 –
Cavallo et al. 2024 24.923 57.492 0.544 – – –
Hunt & Reffert 2023 24.889 57.449 0.538 -0.961 -1.682 –
He et al. 2023 24.936 57.489 0.557 -0.974 -1.681 –

💡 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– 1.7 1.44 1.22 103 -0.060 118 – –
Hunt & Reffert 2024 – – – – – 118(1) – –
Cavallo et al. 2024 1.62 1.34 – 275 -0.060 – – –
Hunt & Reffert 2023 1.70 1.44 1.22 103 – – – –
He et al. 2023 1.70 1.90 – 40 – – – –

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

Visualization

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