8-12 July 2013
Africa/Johannesburg timezone
<a href="http://events.saip.org.za/internalPage.py?pageId=13&confId=32"><font color=#ff0000>SAIP2013 PROCEEDINGS AVAILABLE</font></a>

Development of an Improved Mode Identification Formula For Pulsating Stars

9 Jul 2013, 14:30
20m
Oral Presentation Track D1 - Astrophysics Astro

Speaker

Mr Getachew Mekonnen Mengistie (North West University, Mafikeng Campus)

Abstract content <br> &nbsp; (Max 300 words)

Medupe et al. (2009) developed a new formula for photometric mode identification by considering the shapes of eigen functions in A stars. We calculated opacity tables using ATLAS9 model atmosphere computer program and use this to fit the new formula to delta Scuti stars.
In this talk, I am going to explain and review mode
identification methods for pulsating stars and present the new improved photometric mode identification formula and our results.

Apply to be<br> considered for a student <br> &nbsp; award (Yes / No)?

Yes

Level for award<br>&nbsp;(Hons, MSc, <br> &nbsp; PhD)?

PhD.

Would you like to <br> submit a short paper <br> for the Conference <br> Proceedings (Yes / No)?

No

Main supervisor (name and email)<br>and his / her institution

Thebe Rodney Medupe (thebe@ast.uct.ac.za , thebe@baghayogo.ast.uct.ac.za)
North West University, Mafikeng Campus

Primary author

Mr Getachew Mekonnen Mengistie (North West University, Mafikeng Campus)

Co-author

Prof. Thebe Rodney Medupe (North West University, Mafikeng Campus)

Presentation Materials

There are no materials yet.