CWNU 2151

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0.26 UTI
0.0
CN
0.44
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 2.2 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.44 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2151 is a sparse, loose object of low 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 (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– 341.904 55.551 0.238 -2.571 -2.889 -61.978
Hunt & Reffert 2024 341.932 55.55 0.231 -2.561 -2.891 -61.97
Cavallo et al. 2024 341.824 55.548 0.231 – – –
Hunt & Reffert 2023 341.932 55.55 0.231 -2.561 -2.891 -61.97
He et al. 2023 341.906 55.553 0.25 -2.581 -2.92 –

💡 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– 3.82 1.55 0.62 269 0.450 178 – –
Hunt & Reffert 2024 – – – – – 178(1) – –
Cavallo et al. 2024 4.15 1.20 – 269 0.450 – – –
Hunt & Reffert 2023 3.82 1.68 0.62 220 – – – –
He et al. 2023 3.55 1.55 – 708 – – – –

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

Visualization

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