  We report the first detection of molecular gas beyond redshift 7. The
molecular gas is associated with the host galaxy of the quasar candidate PSO
J145.5964+19.3565 and its companion PSO J145.5964+19.3565N separated by 20.7
kpc. The molecular gas of both companions is detected in two rotational
transition lines of carbon monoxide, CO(6-5) and CO(7-6). We also detected the
Lyman-alpha line of PSO J145.5964+19.3565 at z=7.08. The Lyman-alpha line
emission is extended and might represent the blended emission of two different
sources at a separation of <5 kpc. The detected CO and Lyman-alpha emission
likely originate from a system of interacting star-forming galaxies that might
host a quasar(s). We also report the detection of a new emission line from the
system which is a possible 793.62-GHz water maser line.
