The Trojan Horse Method (THM) is a powerful technique allowing to measure the low-energy trend of the astrophysical S(E)-factor of astrophysically important nuclear reactions. This is because Coulomb barrier is overcome in the entrance channel so it does not prevent the exploration of the astrophysically relevant energy region. In addition, no electron screening affects the low-energy behaviour of the THM S(E)-factor because of such beam energies (of the order of several MeV). In the last few years the THM has been applied to several reactions which are important in different astrophysical scenarios, explosive nucleosynthesis (novae) and quiescent burning (AGB and main sequence stars). In the context of novae nucleosynthesis the 17O(p,a)14N has been measured, the excitation function extending down to zero energy. Preliminary results are discussed. As regards quiescent burning, the preliminary analysis of the 18O(p,a)15N reaction in the 0-250keV energy range is presented, while new results on the 11B(p,a0)8Be are shown in connection with the problem of light element depletion in main sequence stars. These reactions were studied by transferring a virtual proton from a deuteron target. With the same technique neutron induced reactions can be easily studied, by selecting the neutron quasi-free transfer. Results on the 6Li(n,a)3H studied via the 6Li(d,a3H)n are extensively discussed.
*Please note different time.