CWNU 240

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0.25 UTI
0.0
CN
0.61
Cdens
0.12
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 7.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.61 Moderately dense
  • CC3 0.12 Very low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 240 is a sparse, moderately dense object of very low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Relatively close Low 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 – 102.533 0.912 0.785 -1.099 -1.053 29.37
Hunt & Reffert 2024 102.538 0.957 0.761 -1.102 -1.017 29.369
Cavallo et al. 2024 102.544 0.91 0.762 – – –
Hunt & Reffert 2023 102.538 0.957 0.761 -1.102 -1.017 29.369
He et al. 2022 102.536 0.82 0.8 -1.16 -1.05 –

💡 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
Hunt & Reffert 2024 – – – – – 102* – –
Cavallo et al. 2024 1.22 0.89 – 129 -0.050 – – –
Hunt & Reffert 2023 1.23 0.54 0.56 256 – – – –
He et al. 2022 1.12 1.08 – 100 -0.930 – – –

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

Visualization

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