CWNU 128

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0.47 UTI
0.55
CN
0.69
Cdens
0.5
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 10.1 [arcmin]
  • CN 0.55 Moderately populated
  • Cdens 0.69 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 128 is a moderately populated, moderately dense 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.
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 – 117.641 -35.16 0.712 -0.751 -0.074 11.3
Hu & Soubiran 2025 117.62 -35.148 – – – –
Hunt & Reffert 2024 117.695 -35.12 0.701 -0.756 -0.078 3.954
Cavallo et al. 2024 117.62 -35.148 0.697 – – –
Hunt & Reffert 2023 117.695 -35.12 0.701 -0.756 -0.078 3.954
He et al. 2022 117.662 -35.143 0.72 -0.74 -0.11 8.1

💡 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 – – – – -0.080* – – –
Hunt & Reffert 2024 – – – – – 234* – –
Cavallo et al. 2024 1.45 1.24 – 562 0.420 – – –
Hunt & Reffert 2023 1.35 1.31 1.25 293 – – – –
He et al. 2022 1.91 1.56 – 251 0.862 – – –

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

Visualization

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