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Ram-Pressure Induced Star Formation in the LMC

Published online by Cambridge University Press:  05 March 2013

Chiara Mastropietro ,
Andreas Burkert  and
Ben Moore
Chiara Mastropietro*
Affiliation:
Universitäts Sternwarte München, Scheinerstr. 1, D-81679 München, Germany
Andreas Burkert
Affiliation:
Universitäts Sternwarte München, Scheinerstr. 1, D-81679 München, Germany
Ben Moore
Affiliation:
Institute for Theoretical Physics, University of Zürich, CH-8057 Zürich, Switzerland
*
CCorresponding author. Email: chiara@usm.uni-muenchen.de
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Abstract

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We use high-resolution n-body/SPH simulations to study the hydrodynamical interaction between the Large Magellanic Cloud and the hot halo of the Milky Way. We investigate whether the ram-pressure acting on the gaseous disk of the satellite can explain the peculiarities observed in the Hi distribution and the location of the recent star formation activity.

Keywords

galaxies: Magellanic Cloudsmethods: n-body simulations
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 25 , Special Issue 3: The Magellanic System , 2008 , pp. 138 - 148
Copyright
Copyright © Astronomical Society of Australia 2008

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