title: Supernova remnant OH masers: signposts of cosmic collision.
abstract: A supernova explosion, the final death throe of a massive star, creates an expanding bubble of hot gas that overruns up the surrounding medium. When a supernova remnant encounters a dense interstellar cloud, the compression may trigger gravitational collapse and the formation of a new generation of stars. This event can be detected through intense stimulated emission in the 1720-megahertz transition of the hydroxyl radical, OH, which yields unique insights into the physical processes and conditions occurring during the interaction.
authors.affiliation: Research Centre for Theoretical Astrophysics, School of Physics A28, University of Sydney, NSW 2006, Australia. wardle@physics.usyd.edu.au
authors.forename: Mark
authors.initials: M
authors.lastname: Wardle
authors.forename: Farhad
authors.initials: F
authors.lastname: Yusef-Zadeh