Speaker
Prof.
Rodney Medupe
(North West University, Mafikeng Campus)
Description
Medupe et al (2009) presented a new formula for calculating perturbation in flux as a function of wavelength and mode. They suggested that such a formula will be suitable for mode-identification and will be better than currently used formulae because it takes into consideration the shapes of the eigenfunctions in the atmospheres of A stars, and does not depend on many parameters. In this poster we compare the new formula with multicolor photometric data and see how it compares with existing formula.
Primary author
Prof.
Rodney Medupe
(North West University, Mafikeng Campus)
