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The Evolution of Tidal Debris

Published online by Cambridge University Press:  26 May 2016

J. Christopher Mihos
J. Christopher Mihos*
Affiliation:
Case Western Reserve University, Department of Astronomy, Cleveland, OH 44106, USA

Abstract

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Galaxy interactions expel a significant amount of stars and gas into the surrounding environment. I review the formation and evolution of the tidal debris spawned during these collisions, and describe how this evolution depends on the large scale environment in which the galaxies live. In addition to acting as a long-lived tracer of the interaction history of galaxies, the evolution of this material - on both large scales and small - has important ramifications for galactic recycling processes, the feeding of the intracluster light and intracluster medium within galaxy clusters, and the delayed formation of galactic disks and dwarf galaxies.

Information

Type
Part 3. Ejection and Outflow
Information
Symposium - International Astronomical Union , Volume 217: Recycling Intergalactic and Interslettar Matter , 2004 , pp. 390 - 399
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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