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The possibility to describe the astrophysical S-factor of the 4He12Cradiative capture is considered in the potential cluster model at the energyrange 0.1-4.0 MeV. It is shown that the approach used, which takes into accountE2 transitions only, gives a good description of the new experimental data foradjusted parameters of potentials and leads to the value S(300) =16.0$\cdotp$keV b.

Astrophysical S-factor of 4He12C radiative capture at low energies