CWNU 2002

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0.44 UTI
0.27
CN
0.95
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.7 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 0.95 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2002 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Distant High extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 133.644 -42.11 0.33 -5.744 4.863 47.207
Hunt & Reffert 2024 133.661 -42.135 0.338 -5.719 4.831 46.055
Cavallo et al. 2024 133.67 -42.11 0.326 – – –
Hunt & Reffert 2023 133.661 -42.135 0.338 -5.719 4.831 46.055
He et al. 2023 133.642 -42.099 0.345 -5.744 4.867 –

💡 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 – – – – – 844* – –
Cavallo et al. 2024 3.22 3.72 – 302 0.060 – – –
Hunt & Reffert 2023 2.83 3.72 2.73 293 – – – –
He et al. 2023 3.16 3.55 – 891 – – – –

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

Visualization

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