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| Natura: | Preprint |
| Pubblicazione: |
2025
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| Soggetti: | |
| Accesso online: | https://arxiv.org/abs/2502.10493 |
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| _version_ | 1866918126167261184 |
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| author | Miszuda, A. |
| author_facet | Miszuda, A. |
| contents | 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 $M_{\odot}$ $β$ Cephei-type star |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2502_10493 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Pulsational characteristics of mass accreting stars in close binary systems Miszuda, A. Solar and Stellar Astrophysics 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 $M_{\odot}$ $β$ Cephei-type star |
| title | Pulsational characteristics of mass accreting stars in close binary systems |
| topic | Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2502.10493 |