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.
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
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 |
| Dewey Decimal Classification: | 530 Physics |
| Uncontrolled Keywords: | galaxies: Magellanic Clouds — methods: n-body simulations |
| Language: | English |
| Date: | 2008 |
| Deposited On: | 26 Feb 2009 14:17 |
| Last Modified: | 18 Feb 2018 11:05 |
| Publisher: | CSIRO |
| ISSN: | 1323-3580 |
| OA Status: | Closed |
| Publisher DOI: | https://doi.org/10.1071/AS07049 |
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Mastropietro, C