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2011MNRAS.416..601S - Mon. Not. R. Astron. Soc., 416, 601-617 (2011/September-1)
Simulations of the formation and evolution of isolated dwarf galaxies – II. Angular momentum as a second parameter.
SCHROYEN J., DE RIJCKE S., VALCKE S., CLOET-OSSELAER A. and DEJONGHE H.
Abstract (from CDS):
These simulations show that flattening by rotation is key to reproducing the observed characteristics of flat dwarf galaxies, proving particularly efficient in erasing metallicity gradients. We propose a `centrifugal barrier mechanism' as an alternative to the previously suggested `fountain mechanism' for explaining the flat metallicity profiles of dIrrs and flat, rotating dEs. While only flattening the dark matter halo has little influence, the addition of angular momentum slows down the infall of gas, so that star formation (SF) and the ensuing feedback are less centrally concentrated, occurring galaxy-wide. Additionally, this leads to more continuous star formation histories by preventing large-scale oscillations in the star formation rate (`breathing'), and creates low-density holes in the interstellar medium, in agreement with observations of dIrrs.
Our general conclusion is that rotation has a significant influence on the evolution and appearance of dwarf galaxies, and we suggest angular momentum as a second parameter (after galaxy mass as the dominant parameter) in dwarf galaxy evolution. Angular momentum differentiates between SF modes, making our fast rotating models qualitatively resemble dIrrs, which does not seem possible without rotation.
Abstract Copyright: 2011 The Authors Monthly Notices of the Royal Astronomical Society2011 RAS
Journal keyword(s): methods: numerical - galaxies: dwarf - galaxies: evolution - galaxies: formation
Simbad objects: 19
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