CWNU 212

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0.32 UTI
0.25
CN
0.33
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.6 [N/pc2]
  • CN 0.25 Poorly populated
  • Cdens 0.33 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 212 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (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– 120.695 -28.857 0.66 -2.868 3.148 8.798
Hunt & Reffert 2024 120.618 -28.865 0.647 -2.835 3.103 17.44
Cavallo et al. 2024 120.688 -28.819 0.655 – – –
Hunt & Reffert 2023 120.618 -28.865 0.647 -2.835 3.103 17.44
He et al. 2022 120.642 -28.806 0.67 -2.88 3.14 –

💡 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– 1.42 0.19 0.45 193 0.057 137 – –
Hunt & Reffert 2024 – – – – – 137(1) – –
Cavallo et al. 2024 1.48 0.12 – 316 0.350 – – –
Hunt & Reffert 2023 1.42 0.19 0.45 193 – – – –
He et al. 2022 1.38 0.48 – 40 -0.236 – – –

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

Visualization

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