Proc. IAU volume 13, issue S334, P394-395 2017 DOI: 10.1017/s174392131701078x View full text
P. Zivick, N. Kallivayalil, S. Linden, T. Fritz, G. Besla, R. P. van der Marel, S. Kozłowski, M. C. Geha, C. S. Kochanek, J. Anderson, C. R. Alcock

Abstract: AbstractAs new work on the proper motions (PMs) of the Large Magellanic Cloud (LMC) has come out, our view of the history of the Magellanic Clouds has evolved. We now believe they are on their first infall into the Milky Way (MW), having been tidally bound at the start of infall (though not necessarily now). Combining these observations with initial PMs of the Small Magellanic Cloud (SMC) suggests a new formation mechanism of the Magellanic Stream through the stripping of material from the SMC. However, large …

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