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Since the discovery of molecular resonances in $^{12}$C+$^{12}$C in the earlysixties a great deal of research work has been undertaken to study$\alpha$-clustering and resonant effects of the fusion process at sub-Coulombbarrier energies. The modified astrophysical $S^{*}$ factors of$^{12}$C+$^{12}$C fusion have been extracted from direct fusion measurements atdeep sub-barrier energies near the Gamow window. They were also obtained by theindirect Trojan horse method (THM). A comparison of direct measurements and theTHM, which elucidates problems in the analysis of the THM, is discussed in thisLetter to the Editor.

Status on $\mathbf{{}^{12}{\rm C}+{}^{12}{\rm C}}$ fusion at deep subbarrier energies: impact of resonances on astrophysical $S^{*}$ factors