CWNU 89

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0.42 UTI
0.47
CN
0.5
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 11.6 [arcmin]
  • CN 0.47 Poorly populated
  • Cdens 0.5 Moderately dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 89 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Relatively close Low extinction Near-solar metallicity Young

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 – 133.239 -54.426 0.777 -5.717 4.455 13.666
Hunt & Reffert 2024 133.141 -54.446 0.779 -5.692 4.513 16.56
Cavallo et al. 2024 133.211 -54.461 0.783 – – –
Hunt & Reffert 2023 133.141 -54.446 0.779 -5.692 4.513 16.56
He et al. 2022 133.295 -54.428 0.78 -5.68 4.48 –

💡 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 – – – – – 77* – –
Cavallo et al. 2024 1.16 0.11 – 178 0.490 – – –
Hunt & Reffert 2023 1.20 0.32 0.24 54 – – – –
He et al. 2022 1.23 0.54 – 79 0.274 – – –

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

Visualization

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