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The chemistry of the last major merger

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If you have a question about this talk, please contact Francisco Paz-C .

One prediction of ΛCDM is the existence of partially phase-mixed substructures from accreted dwarf galaxies in the Milky Way stellar halo. Recently, the discovery of the Gaia Sausage Enceladus (GSE) has revolutionised our understanding of the complex assembly of the Milky Way halo. We present a review of the chemistry that characterises the last major merger that happened to the Milky Way some 9-10 Gy ago.

This talk is part of the Institute of Astronomy Seminars series.

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MR15, CMS HEP Seminar Room, Cavendish Laboratory Mill Lane Cambridge Lecture Room 7

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