The roAp phenomenon - many unsolved issues

Details The roAp phenomenon - many unsolved issues The roAp phenomenon - many unsolved issues

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008coska..38..301s&link_type=abstract

Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no. 2, p. 301-310.

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Stars: Chemically Peculiar, Stars: Oscillations, Stars: Variables: Other

Scientific paper

Many issues have arisen with the increasing variety of observations of roAp stars. I will discuss the blue-to-red motion in the line profile variation which have recently been found in NdIII and PrIII lines in many roAp stars. To understand the rapid oscillations in Ap stars, the influence of magnetic fields and chemical peculiarity must be taken into account. I will discuss the wave propagation in a stratified plane atmosphere with a magnetic field as fundamental concepts.

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