CWNU 2204

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0.33 UTI
0.0
CN
0.51
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 2.6 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.51 Moderately dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2204 is a sparse, moderately dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by high 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– 341.256 60.739 0.543 -4.165 -2.232 26.403
Hunt & Reffert 2024 341.241 60.641 0.55 -4.165 -2.24 –
Cavallo et al. 2024 341.32 60.745 0.543 – – –
Hunt & Reffert 2023 341.241 60.641 0.55 -4.165 -2.24 –
He et al. 2023 341.301 60.753 0.54 -4.162 -2.22 –

💡 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– 1.79 3.37 1.63 136 0.160 204 – –
Hunt & Reffert 2024 – – – – – 204(1) – –
Cavallo et al. 2024 1.97 2.98 – 178 0.160 – – –
Hunt & Reffert 2023 1.79 3.37 1.63 136 – – – –
He et al. 2023 1.70 3.60 – 14 – – – –

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

Visualization

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