Abstract
An analysis of the times of maximum light of three SX Phe star was carried out. The results support a monotonous decrement of the period which is consistent with the theoretical models of pre-white-dwarfs of 0.2 Mo.Key wordsStarsSX Phe, Delta Scuti starsvariable stars pulsation
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.