In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no. 2
H. Shibahashi
Details:
Year, pages: 2008, 301 - 310
Keywords:
stars: chemically peculiar, stars: oscillations, stars: variables: other
Original source URL: http://www.astro.sk/caosp/Eedition/Abstracts/2008/Vol_38/No_2/pp301-310_abstract.html
About article:
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 Nd III and Pr III 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.
How to cite:
ISO 690:
Shibahashi, H. 2008. The roAp phenomenon - many unsolved issues. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no.2, pp. 301-310. 1335-1842.
APA:
Shibahashi, H. (2008). The roAp phenomenon - many unsolved issues. Contributions of the Astronomical Observatory Skalnaté Pleso, 38(2), 301-310. 1335-1842.