Pulsational characteristics of mass accreting stars in close binary systems
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 Cephei-type star
Cite
@article{arxiv.2502.10493,
title = {Pulsational characteristics of mass accreting stars in close binary systems},
author = {A. Miszuda},
journal= {arXiv preprint arXiv:2502.10493},
year = {2025}
}
Comments
4 pages. Contribution to the conference "Binary and multiple stars in the era of big surveys," Litomysl, CZ, September 2024. Accepted for publication in Contributions of the Astronomical Observatory Skalnate Pleso