CWNU 437

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0.27 UTI
0.29
CN
0.18
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 17.2 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 0.18 Very loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 437 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, below 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)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 124.769 -43.521 0.883 -5.014 4.08 28.645
Hunt & Reffert 2024 124.588 -43.34 0.871 -5.03 4.1 29.186
Cavallo et al. 2024 124.847 -43.529 0.877 – – –
Hunt & Reffert 2023 124.588 -43.34 0.871 -5.03 4.1 29.186
He et al. 2022 124.74 -43.503 0.89 -5.01 4.02 –

💡 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 1.21 1.14 – 58 -0.020 – – –
Hunt & Reffert 2023 1.08 0.90 1.15 38 – – – –
He et al. 2022 0.83 1.14 – 32 -0.642 – – –

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

Visualization

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