The growth of Rh on Au(111) was studied using UHV-STM and Auger electr
on spectroscopy. At room temperature, Volmer-Weber cluster growth was
observed as expected from the surface energies and the immiscibility o
f Rh and Au below 650-degrees-C. After annealing to 400-degrees-C, the
Rh Auger intensity decreased and STM revealed the formation of Au isl
ands on the surface. Atomic-resolution images obtained after annealing
showed a high density of defects due to Rh incorporation within the A
u terraces and beneath the Au islands. The results demonstrate surface
intermixing and growth by surface atom displacement and formation of
substrate islands even for these immiscible systems.