  We observed the X-ray binaries CirX-1, ScoX-1, GRS 1915+105, GX13+1, and
CygX-1 with the Atacama Large Millimeter/submillimeter Array (ALMA). Unresolved
continuum emission is found at the positions of all the sources at a frequency
of 92 GHz, with flux densities ranging between 0.8 and 10 mJy/beam. In all
cases the emission can be associated with jets that have been extensively
observed at lower frequencies. We searched for line emission from H$\alpha$
recombination, SiO,H2O, and CH3OH at the positions of all the sources and, for
CirX-1 and CygX-1, also at regions where shocks associated with an interaction
between the jet and the interstellar medium had previously been observed. The
search did not yield any significant detection, resulting in 3$\sigma$ upper
limits between 0.65 and 3.7 K km s$^{-1}$ for the existence of line emission in
these regions. In contrast, we detected spatially unresolved SiO emission in
the field of view of GX13+1, and we tentatively associate this emission with a
SiO maser in a potential young stellar object or evolved star. We also found
spatially extended line emission at two additional sites in the field of view
of GX13+1 that we tentatively associate with emission from SO and CH3OH; we
speculate that it may be associated with a star-forming region, but again we
cannot rule out alternative origins such as emission from evolved stars.
