Speaker
Mr
Massimo Predieri
(University of the Witwatersrand)
Abstract content <br> (Max 300 words)
The Kepler satellite, launched in March 2009, has by almost uninterrupted observation produced light curves of unprecedented precision. These newly acquired high quality data offer new opportunities for detailed testing of the hydrodynamic processes that drive stellar evolution. Asteroseismology is one of the most important tools for studying stellar structure - by comparing observed pulsations with the predictions of theoretical models. I report on my theoretical study of the effects that tides generated by the companion star have on pulsations in binary star components.
Level for award<br> (Hons, MSc, <br> PhD)?
MSc
Apply to be<br> considered for a student <br> award (Yes / No)?
Yes
Main supervisor (name and email)<br>and his / her institution
Prof. F.A.M Frescura
fabiofrescura@gmail.com
University of the Witwatersrand
Would you like to <br> submit a short paper <br> for the Conference <br> Proceedings (Yes / No)?
No
Primary author
Mr
Massimo Predieri
(University of the Witwatersrand)
