We investigate properties of two-dimensional asymptotically flat black
holes which arise in both string theory and in scale invariant theori
es of gravity. By introducing sources in the field equations we show h
ow such objects can arise as the endpoint of gravitational collapse. W
e also investigate the thermodynamic and quantum properties, which giv
e rise to a fundamental length scale. The 't Hooft prescription for cu
tting off eigenmodes of particle wavefunctions is shown to be source d
ependent, unlike the four-dimensional case. The relationship between t
hese black holes and those considered previously in (1 + 1) dimensions
is discussed.