  An energy deposition of \sim 10^{50} ergs into the exterior 10^{-3} M_\sun
layers of a red giant is calculated to produce an optical phenomenon similar to
afterglows of gamma-ray bursts (GRB) recently observed. This model can be
realized if a GRB is generated by some mechanism in a close binary system. In
contrast to a ``hypernova'' scenario for GRB recently proposed by Paczy\'nski
(1997), this model does not require a huge kinetic energy of the expanding
shell to explain optical afterglows of GRB.
