Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 462, Issue 3, Pages 2418-2430Publisher
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stw1793
Keywords
methods: numerical; galaxies: evolution; galaxies: formation; galaxies: starburst; galaxies: star formation; cosmology: theory
Categories
Funding
- European Research Council through ERC-StG grant [EXAGAL-308037]
- German Science Foundation [SFB-881]
- Danish National Research Foundation
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We introduce the 'Illustris zoom simulation project', which allows the study of selected galaxies forming in the Lambda cold dark matter (Lambda CDM) cosmology with a 40 times better mass resolution than in the parent large-scale hydrodynamical Illustris simulation. We here focus on the starburst properties of the gas in four cosmological simulations of major mergers. The galaxies in our high-resolution zoom runs exhibit a bursty mode of star formation with gas consumption time-scales 10 times shorter than for the normal star formation mode. The strong bursts are only present in the simulations with the highest resolution, hinting that a too low resolution is the reason why the original Illustris simulation showed a dearth of starburst galaxies. Very pronounced bursts of star formation occur in two out of four major mergers we study. The high star formation rates, the short gas consumption time-scales and the morphology of these systems strongly resemble observed nuclear starbursts. This is the first time that a sample of major mergers is studied through self-consistent cosmological hydrodynamical simulations instead of using isolated galaxy models setup on a collision course. We also study the orbits of the colliding galaxies and find that the starbursting gas preferentially appears in head-on mergers with very high collision velocities. Encounters with large impact parameters do typically not lead to the formation of starbursting gas.
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