The gravitational and hydrodynamical interaction between the Large Magellanic Cloud and the Galaxy

By C. Mastropietro, B. Moore, Lucio Mayer, James Wadsley, J. W. U. O. Zurich, McMaster University. 2004

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We use high-resolution N-body/smoothed particle hydrodynamic simulations to study the hydrodynamical and gravitational interaction between the Large Magellanic Cloud (LMC) and the Milky Way Galaxy. We model the dark and hot extended halo components as well as the stellar/gaseous discs of the two galaxies. Both galaxies are embedded in extended cuspy �CDM dark matter haloes. We follow the previous 4 Gyr of the LMC’s orbit such that it ends up with the correct location and orientation on the sky. Tidal forces elongate the LMC’s disc, forcing a bar and creating a strong warp and diffuse stellar halo, although very few stars become unbound. The stellar halo may account for some of the microlensing events observed towards the LMC. Ram pressure from a low-density ionized halo is then sufficient to remove

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/f69184fb3980a8e88360530b91112b5db9dee7a5

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