CWNU 2409

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0.33 UTI
0.0
CN
0.52
Cdens
0.5
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 3.3 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.52 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2409 is a sparse, moderately dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It was recently reported in the literature.
Relatively close Low extinction Near-solar metallicity Old

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 – 122.54 -25.744 0.316 -5.221 5.06 69.966
Hu & Soubiran 2025 122.539 -25.769 – – – –
Hunt & Reffert 2024 122.547 -25.746 0.317 -5.214 5.049 62.207
Cavallo et al. 2024 122.539 -25.769 0.318 – – –
Hunt & Reffert 2023 122.547 -25.746 0.317 -5.214 5.049 62.207
He et al. 2023 122.555 -25.75 0.328 -5.207 5.046 69.27

💡 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 – – – – -0.140* – – –
Hunt & Reffert 2024 – – – – – 88* – –
Cavallo et al. 2024 2.57 0.31 – 1622 0.060 – – –
Hunt & Reffert 2023 2.81 0.21 0.72 940 – – – –
He et al. 2023 2.82 0.25 – 1413 – – – –

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

Visualization

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