English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

Eclipsing binary systems with pulsating components offer a unique possibilityto accurately measure the most important parameters of pulsating stars, tostudy their evolution, and to test the pulsation theory. I will show what wecan learn about the pulsating stars from the analysis of such systems and howwe can do it. Special attention will be paid to the mass, radius, p-factor, anddistance determination. Although the core of the method is based on theobservations of double-lined eclipsing spectroscopic binaries, with the help ofthe pulsation theory, it is possible to measure absolute parameters forsingle-lined binaries also.

Cepheids in Eclipsing Binaries. What and How We Can Learn About Them