  We investigate the dynamical effects of rapid gas expulsion from the core of
a young stellar cluster. The aims of this study are to determine 1) whether a
mass-segregated core survives the gas expulsion and 2) the probable location of
any massive stars that have escaped from the core. Feedback from massive stars
is expected to remove the gas from the core of the cluster first, as that is
where most massive stars are located. We find that gas expulsion has little
effect on the core for a core star formation efficiency, of greater than 50%.
For lower values of star formation efficiency down to 20%, a reduced core
survives containing the majority of the massive stars while some of them are
dispersed into the rest of the cluster. In fact we find that ejected stars
migrate from radial to tangential orbits due to stellar encounters once they
leave the core. Thus, the location of massive stars outside of the core does
not exclude their forming in the dense cluster core. Few massive stars are
expected to remain in the core for a star formation efficiency lower than 20%.
