IALP 13078
INSTITUTO DE ASTROFISICA LA PLATA
Unidad Ejecutora - UE
artículos
Título:
A 3-D look into the atmosphere?
Revista:
Highlights of Astronomy
Editorial:
Cambridge Journals
Referencias:
Lugar: Cambridge; Año: 2010 vol. 15 p. 151 - 160
ISSN:
0080-1372
Resumen:
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 relatedstars. It is divided into 3 sections: Magnetic field and surface structures, Pulsations in the atmospheres of roAp stars/inversions, and Spectral synthesis/atmospheric models.
