Mastropietro, C; Burkert, A; Moore, B (2008). Ram-pressure induced star formation in the LMC. Publications of the Astronomical Society of Australia, 25(3):138-148.
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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
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|Item Type:||Journal Article, refereed, original work|
|Communities & Collections:||07 Faculty of Science > Institute for Computational Science|
|Uncontrolled Keywords:||galaxies: Magellanic Clouds — methods: n-body simulations|
|Deposited On:||26 Feb 2009 14:17|
|Last Modified:||27 Nov 2013 22:41|
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