We examine, as model-independently as possible, the production of bileptons
at hadron colliders. When a particular model is necessary or useful, we ch
oose the 3-3-1 model. We consider a variety of processes: q (q) over bar --
>Y++Y--, u (d) over bar-->Y++Y-, (u) over bar d-->Y+Y--, q (q) over bar-->Y
(++)e(-)e(-), q (q) over bar-->phi(++)phi(--), u (d) over bar-->phi(++)phi(
-), and (u) over bar d -->phi(+)phi(--), where Y and phi are vector and sca
lar bileptons, respectively. Given the present low-energy constraints, we f
ind that, at the Fermilab Tevatron, vector bileptons are unobservable, whil
e Light scalar bileptons (M(phi)less than or similar to 300 GeV) are just b
arely observable. At the CERN LHC, the reach is extended considerably: vect
or bileptons of mass M(Y)less than or similar to 1 TeV are observable, as a
re scalar bileptons of mass M(phi)less than or similar to 850 GeV. [S0556-2
821(99)05205-4].