CWNU 538

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0.31 UTI
0.31
CN
0.25
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 10.8 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 0.25 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 538 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied 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 – 117.541 -30.864 0.633 -4.298 4.463 8.634
Hunt & Reffert 2024 117.508 -30.942 0.635 -4.288 4.5 22.184
Cavallo et al. 2024 117.443 -30.79 0.635 – – –
Hunt & Reffert 2023 117.508 -30.942 0.635 -4.288 4.5 22.184
He et al. 2022 117.541 -30.898 0.63 -4.3 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
Hunt & Reffert 2024 – – – – – 140* – –
Cavallo et al. 2024 1.54 1.35 – 76 0.140 – – –
Hunt & Reffert 2023 1.48 1.34 2.41 34 – – – –
He et al. 2022 1.66 1.74 – 25 0.457 – – –

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

Visualization

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