A 3-D look into the atmosphere?

Warning

This publication doesn't include Faculty of Economics and Administration. It includes Faculty of Science. Official publication website can be found on muni.cz.
Authors

WADE GA. MASHONKINA L. RYABCHIKOVA T. KRTIČKA Jiří SILVESTER J. KOCHUKHOV O. SOUSA JC. NOMURA T. WAHLGREN GM. GRUBERBAUER M. HUBRIG S. BRIQUET M. YUCE K. DRAKE N. NUNEZ N. GRAY RO. ŽIŽNOVSKÝ Jozef COWLEY C. SHAVRINA A. DWORETSKY M. PINTADO O. POLOSUKHINA N. CIDALE L.

Year of publication 2010
Type Article in Proceedings
Conference Highlights of Astronomy
MU Faculty or unit

Faculty of Science

Citation
Web http://journals.cambridge.org/action/displayAbstract?fromPage=online&aid=7915275
Doi http://dx.doi.org/10.1017/S1743921310008550
Field Astronomy and astrophysics
Keywords stars: chemically peculiar stars: atmospheres stars: variables: roAp stars stars: magnetic fields
Description The atmospheres of chemically peculiar stars can be highly structured in both the horizontal and vertical dimensions. While most prevalent in the magnetic stars, these structures can also exist in non-magnetic stars. In addition to providing an important window to understanding the physical processes at play in these complex atmospheres, they can also be exploited to study stellar pulsations. This article reviews contributions to the session "A 3D look into the atmosphere" of the Joint Discussion "Progress in understanding the physics of Ap and related stars". It is divided into 3 sections: "Magnetic field and surface structures", "Pulsations in the atmospheres of roAp stars/inversions", and "Spectral synthesis/atmospheric models".
Related projects:

You are running an old browser version. We recommend updating your browser to its latest version.