CWNU 1580

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0.45 UTI
0.31
CN
0.68
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 3.4 [N/pc2]
  • CN 0.31 Poorly populated
  • Cdens 0.68 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1580 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, above 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– 182.17 -60.003 0.395 -7.3 0.273 -21.885
Hunt & Reffert 2024 182.068 -59.978 0.389 -7.295 0.284 -21.813
Cavallo et al. 2024 182.17 -60.004 0.39 – – –
Hunt & Reffert 2023 182.068 -59.978 0.389 -7.295 0.284 -21.813
He et al. 2023 182.196 -60.004 0.396 -7.296 0.271 –

💡 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– 2.36 1.48 0.66 117 -0.150 220 – –
Hunt & Reffert 2024 – – – – – 220(1) – –
Cavallo et al. 2024 2.15 1.59 – 117 -0.150 – – –
Hunt & Reffert 2023 2.36 1.48 0.66 72 – – – –
He et al. 2023 2.40 1.35 – 251 – – – –

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

Visualization

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