I study the time-symmetric initial-data problem in theories with a mas
sless scalar field (dilaton), free or coupled to a Maxwell held in the
stringy way, finding different initial-data sets describing an arbitr
ary number of black holes with arbitrary masses, charges, and asymptot
ic value of the dilaton. The presence of the scalar held gives rise to
a number of interesting effects. The mass and charges of a single bla
ck hole are different in its two asymptotically hat regions across the
Einstein-Rosen bridge. The same happens to the value of the dilaton a
t infinity. This forbids the identification of these asymptotic region
s in order to build (Misner) wormholes in the most naive way. Using di
fferent techniques, I find regular initial data for stringy wormholes.
The price paid is the existence singularities in the dilaton held. Th
e presence of a single-valued scalar seems to constrain strongly the a
llowed topologies of the initial spacelike surface. Other kinds of sca
lar fields (taking values on a circle or being defined up to an additi
ve constant) are also briefly considered.