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arXiv · 2502.10493

Pulsational characteristics of mass accreting stars in close binary systems

A. Miszuda
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Abstract

Eclipsing binaries with pulsating components are a distinct subclass of binaries, merging orbital and pulsational analyses. In recent years, that subclass led to the definition of a newly formed branch of tidal asteroseismology. While single-star pulsators are well understood, the effects of binarity and possible mass transfer on pulsational characteristics, particularly in mass-gaining stars, remain to be systematically explored. Here, I present preliminary results on the asteroseismic properties of a mass-accreting model for a 10 $M_{\odot}$ $\beta$ Cephei-type star

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A. Miszuda. 2025-02-14. Pulsational characteristics of mass accreting stars in close binary systems. https://doi.org/10.31577/caosp.2025.55.3.196

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