Rigging dark halos: why is hierarchical galaxy formation consistent with the inside-out build-up of...
Rigging dark halos: why is hierarchical galaxy formation consistent with the inside-out build-up of thin discs?
About this item
Full title
Author / Creator
Pichon, C , Pogosyan, D , Kimm, T , Slyz, A , Devriendt, J and Dubois, Y
Publisher
Ithaca: Cornell University Library, arXiv.org
Journal title
Language
English
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Publication information
Publisher
Ithaca: Cornell University Library, arXiv.org
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Scope and Contents
Contents
State-of-the-art hydrodynamical simulations show that gas inflow through the virial sphere of dark matter halos is focused (i.e. has a preferred inflow direction), consistent (i.e. its orientation is steady in time) and amplified (i.e. the amplitude of its advected specific angular momentum increases with time). We explain this to be a consequence...
Alternative Titles
Full title
Rigging dark halos: why is hierarchical galaxy formation consistent with the inside-out build-up of thin discs?
Authors, Artists and Contributors
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Record Identifier
TN_cdi_proquest_journals_2082153136
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2082153136
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.1105.0210
