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Permanent URL to this publication: http://dx.doi.org/10.5167/uzh-30869

Agertz, O; Teyssier, R; Moore, B (2009). Disc formation and the origin of clumpy galaxies at high redshift. Monthly Notices of the Royal Astronomical Society, 397(1):L64-L68.

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Observations of high-redshift galaxies have revealed a multitude of large clumpy rapidly star-forming galaxies. Their formation scenario and their link to present-day spirals are still unknown. In this Letter, we perform adaptive mesh refinement simulations of disc formation in a cosmological context that are unrivalled in terms of mass and spatial resolution. We find that the so-called 'chain-galaxies' and 'clump-clusters' are a natural outcome of early epochs of enhanced gas accretion from cold dense streams as well as tidally and ram-pressured stripped material from minor mergers and satellites. Through interaction with the hot halo gas, this freshly accreted cold gas settles into a large disc-like system, not necessarily aligned to an older stellar component, that undergoes fragmentation and subsequent star formation, forming large clumps in the mass range 107–109 M⊙ . Galaxy formation is a complex process at this important epoch when most of the central baryons are being acquired through a range of different mechanisms – we highlight that a rapid mass loading epoch is required to fuel the fragmentation taking place in the massive arms in the outskirts of extended discs, an accretion mode that occurs naturally in the hierarchical assembly process at early epochs.


142 citations in Web of Science®
139 citations in Scopus®
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Additional indexing

Item Type:Journal Article, refereed, original work
Communities & Collections:07 Faculty of Science > Institute for Computational Science
Dewey Decimal Classification:530 Physics
Uncontrolled Keywords:galaxies: evolution; galaxies: formation; galaxies: haloes
Date:July 2009
Deposited On:26 Feb 2010 13:29
Last Modified:05 Apr 2016 13:56
Additional Information:The attached file is a preprint (accepted version) of an article published in Monthly Notices of the Royal Astronomical Society. The definitive version is available at www3.interscience.wiley.com
Publisher DOI:10.1111/j.1745-3933.2009.00685.x
Related URLs:http://arxiv.org/abs/0901.2536

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