Bimodality of [α Fe]–[Fe/H] distributions is a natural outcome of dissipative collapse and disc growth in Milky Way-type galaxies
Sergey Khoperskov(Centre National de la Recherche Scientifique), Peter Berczik(National Academy of Sciences of Ukraine), S. А. Naroenkov(Russian Academy of Sciences), E. O. Vasiliev(P.N. Lebedev Physical Institute of the Russian Academy of Sciences), Owain Snaith(Centre National de la Recherche Scientifique), M. Haywood(Centre National de la Recherche Scientifique), P. Di Matteo(Observatoire de Paris), M. D. Lehnert(Centre National de la Recherche Scientifique)
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