Abstract
The physics that drive the evolution of O-type stars are not well understood. These stars experience a plethora of different phenomena which alter their evolution, including pulsations, chemical transport, wind mass-loss, rapid rotation, multiplicity, etc. In this chapter, we investigate the diverse variability observed in the massive O+B eclipsing binary HD 165246. We make use of space-based photometry assembled with the K2 mission as well as ground-based spectroscopy to characterise the pulsational variability observed in HD 165246.
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Johnston, C. (2021). The O+B Eclipsing Binary HD 165246. In: Interior Modelling of Massive Stars in Multiple Systems. Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-030-66310-0_3
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