CWNU 1558

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0.49 UTI
0.33
CN
0.88
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.2 [arcmin]
  • CN 0.33 Poorly populated
  • Cdens 0.88 Dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1558 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate 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 – 296.753 28.832 0.341 -2.723 -5.454 21.447
Hunt & Reffert 2024 296.75 28.81 0.344 -2.718 -5.467 –
Cavallo et al. 2024 296.714 28.814 0.343 – – –
Hunt & Reffert 2023 296.75 28.81 0.344 -2.718 -5.467 –
He et al. 2023 296.753 28.83 0.357 -2.718 -5.445 –

💡 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 – – – – – 168* – –
Cavallo et al. 2024 2.17 1.29 – 145 -0.200 – – –
Hunt & Reffert 2023 2.66 1.13 0.56 93 – – – –
He et al. 2023 2.63 1.40 – 25 – – – –

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

Visualization

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