Toward $ab\,initio$ extremely metal poor stars

Extremely metal poor stars have been the focus of much recent attention owing to the expectation that their chemical abundances can shed light on the metal and dust yields of the earliest supernovae. We present our most realistic simulation to date of the astrophysical pathway to the first metal enr...

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Hauptverfasser: Ritter, Jeremy S, Safranek-Shrader, Chalence, Milosavljevic, Milos, Bromm, Volker
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Sprache:eng
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