CWNU 58

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0.49 UTI
0.69
CN
0.62
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 20.8 [arcmin]
  • CN 0.69 Moderately populated
  • Cdens 0.62 Moderately dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 58 is a moderately populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.
Close High extinction Near-solar metallicity Very 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 – 342.006 60.669 1.14 -0.282 -2.44 -14.226
Hunt & Reffert 2024 342.159 60.541 1.134 -0.21 -2.4 -27.477
Cavallo et al. 2024 341.908 60.701 1.142 – – –
Hunt & Reffert 2023 342.159 60.541 1.134 -0.21 -2.4 -27.477
He et al. 2022 341.899 60.908 1.15 -0.5 -2.49 –

💡 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 – – – – – 160* – –
Cavallo et al. 2024 0.91 3.19 – 14 -0.100 – – –
Hunt & Reffert 2023 0.85 3.11 1.69 8 – – – –
He et al. 2022 1.07 1.02 – 1 -0.419 – – –

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

Visualization

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