CWNU 1860

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0.41 UTI
0.31
CN
0.59
Cdens
0.5
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 4.1 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 0.59 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1860 is a poorly populated, moderately dense object of intermediate 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, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity Intermediate age

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 – 341.15 57.041 0.369 -4.285 -3.072 -45.422
Hu & Soubiran 2025 341.159 57.053 – – – –
Hunt & Reffert 2024 341.138 57.053 0.366 -4.29 -3.07 -45.381
Cavallo et al. 2024 341.159 57.053 0.366 – – –
Hunt & Reffert 2023 341.138 57.053 0.366 -4.29 -3.07 -45.381
He et al. 2023 341.182 57.062 0.372 -4.274 -3.056 -45.42

💡 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] Bfr BSS
Hu & Soubiran 2025 – – – – -0.030* – – –
Hunt & Reffert 2024 – – – – – 182* – –
Cavallo et al. 2024 2.42 1.24 – 912 0.520 – – –
Hunt & Reffert 2023 2.74 1.29 0.43 1109 – – – –
He et al. 2023 2.63 1.80 – 631 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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