In this article, we continue A. Labeyrie's work concerning the detecti
on of Gravitational Waves through the deformations of optical wavefron
ts. We give the analytical expressions of the wavefront distortions. S
pecial attention is paid to the discussion of this approach with respe
ct to other works. The wavefront distortions are expected to cause a s
cintillation effect for a distant observer. The observability of this
effect is discussed in the cases of binary stars and millisecond pulsa
rs. It seems unobservable for a single monochromatic source of gravita
tional waves.