Abstract
This chapter serves as a revision of the monograph. We give a brief overview of the work presented in this monograph before musing the future direction of this work. We introduce a number of ideal targets for future application of the methodology presented throughout this work. Finally, we aggregate the inferred core mass estimates obtained throughout this work and place them on a single plot. This plot will serve as a future means of assessing the growth of core masses due to internal chemical mixing and acts as a unifying tool for investigation which does not rely on a particular implementation of a internal chemical mixing mechanism.
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Johnston, C. (2021). Final Remarks. In: Interior Modelling of Massive Stars in Multiple Systems. Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-030-66310-0_8
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DOI: https://doi.org/10.1007/978-3-030-66310-0_8
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