Stellar Exotica produced from Stellar Encounters

The importance of stellar encounters in producing stellar exotica in dense stellar clusters is reviewed. We discuss how collisions between main–sequence stars may be responsible for the production of blue stragglers in globular clusters. We also discuss the possible pathways to the production of X–ray binaries, cataclysmic variables, and millisecond pulsars in globular clusters. Neutron stars in globular clusters are likely to exchange into binaries containing moderate–mass main–sequence stars, replacing the lower–mass components of the original systems. These binaries will become intermediate–mass X–ray binaries (IMXBs), once the moderate–mass star evolves off the main–sequence, as mass is transferred onto the neutron star possibly spinning it up in the process. Such systems may be responsible for the population of millisecond pulsars (MSPs) that has been observed in globular clusters. Additionally, the period of mass– transfer (and thus X–ray visibility) in the vast majority of such systems will have occurred 5 – 10 Gyr ago thus explaining the observed relative paucity of X–ray binaries today, given the large MSP population.