arXiv · astro-ph/9811242
Mergers and Galaxy Assembly
Abstract
Theoretical considerations and observational data support the idea that mergers were more frequent in the past. At redshifts z = 2 to 5, violent interactions and mergers may be implicated by observations of Lyman-break galaxies, sub-mm starbursts, and active galactic nuclei. Most stars in cluster ellipticals probably formed at such redshifts, as did most of the halo and globular clusters of the Milky Way; these events may all be connected with mergers. But what kind of galaxies merged at high redshifts, and are present-epoch mergers useful guides to these early collisions? I will approach these questions by describing ideas for the formation of the Milky Way, elliptical galaxies, and systems of globular clusters.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Joshua E. Barnes. 1998-11-16. Mergers and Galaxy Assembly. https://doi.org/10.1063/1.58601
Cite the original work for its findings. Save a collection to share your selection of sources.