The Ne-22(L-6, d) alpha-transfer reaction has been used to search for
alpha-unbound levels in Mg-26 of importance for resonant alpha-capture
on Ne-22 in stellar helium burning. To determine the resonance streng
ths of the observed states the Ne-22(alpha, n)Mg-25 reaction was inves
tigated in the energy range between 600 and 900 keV. One resonance was
identified and its strength determined. The astrophysical implication
s of the present results are discussed.