CWNU 205

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0.28 UTI
0.0
CN
0.3
Cdens
0.5
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 1.5 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.3 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 205 is a sparse, loose 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 metallicity parameter (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– 93.625 2.834 0.687 0.449 -2.298 5.533
Zhang et al. 2024 93.608 2.846 – – – –
Hunt & Reffert 2024 93.608 2.846 0.643 0.443 -2.308 18.146
Cavallo et al. 2024 93.712 2.772 0.65 – – –
Hunt & Reffert 2023 93.608 2.846 0.643 0.443 -2.308 18.146
He et al. 2022 93.642 2.804 0.69 0.48 -2.31 –

💡 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– 1.52 1.26 1.66 468 0.100 260 – –
Zhang et al. 2024 – – – – -0.179(1) – – –
Hunt & Reffert 2024 – – – – – 260(1) – –
Cavallo et al. 2024 1.52 1.42 – 468 0.100 – – –
Hunt & Reffert 2023 1.42 1.21 1.66 185 – – – –
He et al. 2022 1.74 1.26 – 501 0.916 – – –

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

Visualization

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