CWNU 433

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0.34 UTI
0.25
CN
0.47
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 7.2 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.47 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 433 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 low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Relatively close Low extinction Near-solar metallicity Intermediate age

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 – 125.84 -37.001 0.645 -3.429 3.362 -4.269
Hunt & Reffert 2024 125.845 -37.094 0.641 -3.427 3.367 -2.358
Cavallo et al. 2024 125.73 -36.914 0.641 – – –
Hunt & Reffert 2023 125.845 -37.094 0.641 -3.427 3.367 -2.358
He et al. 2022 125.81 -37.005 0.64 -3.41 3.36 29.3

💡 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 – – – – – 115* – –
Cavallo et al. 2024 1.51 0.43 – 324 0.240 – – –
Hunt & Reffert 2023 1.49 0.40 0.28 113 – – – –
He et al. 2022 1.23 0.48 – 794 -0.930 – – –

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

Visualization

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