CWNU 2206

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0.40 UTI
0.0
CN
0.75
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 3.7 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.75 Dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2206 is a sparse, dense object of high C3 quality. Its parallax locates it at a moderate 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– 75.036 34.393 0.229 0.351 -1.054 –
Hunt & Reffert 2024 75.035 34.379 0.236 0.345 -1.046 –
Cavallo et al. 2024 75.025 34.393 0.228 – – –
Hunt & Reffert 2023 75.035 34.379 0.236 0.345 -1.046 –
He et al. 2023 75.031 34.389 0.241 0.355 -1.028 –

💡 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– 4.27 2.41 1.31 129 0.270 393 – –
Hunt & Reffert 2024 – – – – – 393(1) – –
Cavallo et al. 2024 4.41 2.41 – 129 0.270 – – –
Hunt & Reffert 2023 3.86 2.34 1.31 188 – – – –
He et al. 2023 4.27 2.85 – 10 – – – –

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

Visualization

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