Abstract
The \(\delta \) Sct stars are by far the most common type of pulsating stars at spectral type A. In this, the most extensive review of \(\delta \) Sct stars in the Kepler era, the following topics are discussed: the \(\delta \) Sct instability strip; pulsation amplitudes and frequency ranges of the class; mode selection and identification; and the influence of rotation, evolution, and metallicity on pulsation. The \(\gamma \) Dor variables and the overlap of their instability strip with the \(\delta \) Sct instability strip are outlined, before a short description of especially interesting case-studies is presented, pointing to further reading.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.