In this work we address contributions from scalars to (g-2)(mu). In order t
o explain the recently measured deviation by the BNL experiment on (g-2)(mu
), it is necessary that these scalars are either light or couple strongly w
ith muons. Here we explore this last possibility. We show that a scalar wit
h mass of the order of 10(2) GeV provides significant contribution to (g-2)
(mu) if the Yukawa coupling is about 10(-1). We suggest scenarios where thi
s comes about naturally.