Abstract
To date, magnetic fields have been detected in various types of pulsating stars. For several of these stars, the variability of the magnetic field with their radial pulsation period was confirmed. The physical mechanism of the pulsation variability of the magnetic field remains unknown. We discuss the current state of the problem of magnetic field variability over pulsation cycles in radially pulsating stars.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: 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.
