In this study, led by Roberto Silvotti of the Torino Astrophysical Observatory and published in Monthly Notices of the Royal Astronomical Society (https://ui.adsabs.harvard.edu/abs/2019MNRAS.489.4791S/abstract), we analyze the light curve of a pulsating star that shows very peculiar pulsation modes, which will allow us to reconstruct the internal structure of the star with an accuracy never achieved before.

More details on Media Inaf (https://www.media.inaf.it/2019/09/12/silvotti-piccola-stella-antica/).