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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

Item Type:Journal Article, refereed, original work
Communities & Collections:07 Faculty of Science > Institute for Computational Science
DDC:530 Physics
Uncontrolled Keywords:galaxies: Magellanic Clouds — methods: n-body simulations
Deposited On:26 Feb 2009 14:17
Last Modified:27 Nov 2013 22:41
Publisher DOI:10.1071/AS07049
Citations:Web of Science®. Times Cited: 2
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Scopus®. Citation Count: 2

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