In the book Quantum Gravity in 2+1 dimension by S. Carlip, in the second chapter (section 2.1), he comments that a compact 3-manifold with a flat time orientable Lorentzian metric and a purely spacelike boundary, necessarily has the topology $[0,1]\times \Sigma$, where $\Sigma$ is a closed surface that is homeomorphic to one of the boundary components.
Does this mean that all spacetime manifolds (flat) that we could allow in 2+1 dimension are necessarily of this topology (it seems to be a big restriction)?
Also, is it necessary for the boundary of a spacetime (for those that would have one) to be spacelike ? I have a rough argument (which I am not sure about) for this, that if we had a timelike boundary, in some coordinate system, we would have the boundary at some given value for the space co-ordinates which seems weird to me.