CWNU 80

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0.39 UTI
0.31
CN
0.49
Cdens
0.5
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 15.9 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 0.49 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 80 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Close Low extinction Low mass 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 – 93.855 11.945 1.3 -1.913 -4.505 11.231
Zhang et al. 2024 93.96 11.891 – – – –
Hunt & Reffert 2024 93.96 11.891 1.293 -1.844 -4.497 5.246
Cavallo et al. 2024 93.424 12.373 1.292 – – –
Hunt & Reffert 2023 93.96 11.891 1.293 -1.844 -4.497 5.246
He et al. 2022 93.779 11.874 1.28 -1.91 -4.46 –

💡 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
Zhang et al. 2024 – – – – 0.026* – – –
Hunt & Reffert 2024 – – – – – 49* – –
Cavallo et al. 2024 0.80 0.44 – 112 0.110 – – –
Hunt & Reffert 2023 0.74 0.30 1.07 123 – – – –
He et al. 2022 0.78 0.42 – 63 0.457 – – –

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

Visualization

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