In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 48, no. 1
J. Klevas - A. Kučinskas - S. Wedemeyer - H.-G. Ludwig
Details:
Year, pages: 2018, 280 - 281
Keywords:
stars: atmospheres, convection, hydrodynamics, magnetohydrodynamics (MHD), stars: late-type
Original source URL: http://www.astro.sk/caosp/Eedition/Abstracts/2018/Vol_48/No_1/pp280-281_abstract.html
About article:
We use 3D magnetohydrodynamic CO5BOLD model atmospheres to study the interplay between magnetic fields and convection in the atmospheres of red giant stars. We find that vortex-like structures occur prominently in stars with stronger magnetic fields and lead to alterations of their thermal structures.
How to cite:
ISO 690:
Klevas, J., Kučinskas, A., Wedemeyer, S., Ludwig, H. 2018. Impact of magnetic fields on the structure of convective atmospheres of red giant stars. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 48, no.1, pp. 280-281. 1335-1842.
APA:
Klevas, J., Kučinskas, A., Wedemeyer, S., Ludwig, H. (2018). Impact of magnetic fields on the structure of convective atmospheres of red giant stars. Contributions of the Astronomical Observatory Skalnaté Pleso, 48(1), 280-281. 1335-1842.