Non-Radial Pulsations of Distorted Stellar Structures: Effect of Mass Variation

Eigen-frequencies (EF) of non–radial modes (NRM) of pulsations of differentially rotating (D R) and tidally distorted (T D) stellar models by considering the effect of mass variation (MV) on its equi-potentials surfaces inside a star. The method utilizes an averaging proposal of Kippenhahn and Thoma...

Full description

Bibliographic Details
Main Authors: Seema Saini, Sunil Kumar, Vineet Bhatt, Pradeep Bedi
Format: Article
Language:English
Published: International Journal of Mathematical, Engineering and Management Sciences 2021-10-01
Series:International Journal of Mathematical, Engineering and Management Sciences
Subjects:
Online Access:https://www.ijmems.in/cms/storage/app/public/uploads/volumes/84-IJMEMS-21-0116-6-5-1391-1405-2021.pdf

Similar Items