CWNU 1554

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0.28 UTI
0.0
CN
0.17
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 0.9 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.17 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1554 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low 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– 107.884 -9.159 0.316 -2.056 2.079 68.117
Hunt & Reffert 2024 107.872 -9.191 0.306 -2.003 2.044 77.06
Cavallo et al. 2024 107.908 -9.242 0.309 – – –
Hunt & Reffert 2023 107.872 -9.191 0.306 -2.003 2.044 77.06
He et al. 2023 107.865 -9.132 0.351 -2.08 2.084 68.12

💡 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– 2.95 0.82 2.3 145 0.210 283 – –
Hunt & Reffert 2024 – – – – – 283(1) – –
Cavallo et al. 2024 3.03 0.87 – 145 0.210 – – –
Hunt & Reffert 2023 2.80 0.82 2.30 196 – – – –
He et al. 2023 2.95 0.80 – 79 – – – –

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

Visualization

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