The driving mechanism of roAp stars

Details The driving mechanism of roAp stars The driving mechanism of roAp stars

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008jphcs.118a2052d&link_type=abstract

Journal of Physics: Conference Series, Volume 118, Issue 1, pp. 012052 (2008).

Physics

1

Scientific paper

We analyse in detail the driving mechanism of roAp stars and present the theoretical instability strip predicted by our models with solar metallicity. A particular attention is given to the interpretation of the role played by the different eigenfunctions in the stabilization of the modes at the red edge of the instability strip. The gradient of temperature in the HI opacity bump appears to play a major role in this context. We also consider the particular and complex role played by the shape of the eigenfunctions (location of the nodes, ...).

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