Variations in α-element Ratios Trace the Chemical Evolution of the Disk
It is well established that the chemical structure of the Milky Way exhibits a bimodality with respect to the α -enhancement of stars at a given [Fe/H]. This has been studied largely based on a bulk α abundance, computed as a summary of several individual α -elements. Inspired by the expected subtle...
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Published in | The Astrophysical journal Vol. 883; no. 1; p. 34 |
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Main Authors | , , , , |
Format | Journal Article |
Language | English |
Published |
Philadelphia
IOP Publishing
20.09.2019
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Subjects | |
Online Access | Get full text |
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