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

J. Klevas - A. Kučinskas - S. Wedemeyer - H.-G. Ludwig

Detaily:

Rok, strany: 2018, 280 - 281

Kľúčové slová:

stars: atmospheres, convection, hydrodynamics, magnetohydrodynamics (MHD), stars: late-type

URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2018/Vol_48/No_1/pp280-281_abstract.html

Full text

O článku:

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.

Ako citovať:

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.