of the Al 26 abundance in massive stars. The aim of this work is to report on a direct and
simultaneous measurement of these astrophysically important reactions using an active
target system. The reactions were investigated in inverse kinematics using He 4 as the
active target gas in the detector. We measured the excitation functions in the energy range of
about 2 to 6 MeV in the center of mass. We have found that the cross sections of the Na 23 …