In modern technicolor models, there exist very narrow spin-zero and sp
in-one neutral technihadrons - pi(T)(0),( )rho(T)(0), and omega(T )- w
ith masses of a few 100 GeV. The large coupling of pi(T)(0 )mu(+)mu(-)
, the direct coupling of rho(T)(0) and omega(T) to the photon and Z(0)
, and the superb energy resolution of the First Muon Collider may make
it possible to resolve these technihadrons and produce them at extrao
rdinarily large rates.