OC 0432

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0.51 UTI
0.31
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 5.2 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0432 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Relatively close Low 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 – 116.679 -31.322 0.66 -4.187 4.642 20.599
Hunt & Reffert 2024 116.628 -31.31 0.662 -4.175 4.648 20.606
Cavallo et al. 2024 116.654 -31.308 0.659 – – –
Hunt & Reffert 2023 116.628 -31.31 0.662 -4.175 4.648 20.606
Hao et al. 2022 116.661 -31.308 0.655 -4.106 4.603 –

💡 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 – – – – – 81* – –
Cavallo et al. 2024 1.43 0.67 – 46 -0.020 – – –
Hunt & Reffert 2023 1.44 0.70 0.97 46 – – – –
Hao et al. 2022 – 0.29 – 32 0.370 – – –

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

Visualization

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