Stellar Winds in Single and Binary Star Systems

Autor(en)
Colin Johnstone, Manuel Güdel, Theresa Lüftinger, Dmitry Bisikalo, Andrey Zhilkin, Elke Pilat-Lohinger
Abstrakt

Young low-mass stars are continuously losing mass in the form of stellar

winds. These winds can influence the evolution of the atmospheres of

planets that orbit these stars. Supersonic winds from the parent star

compress the planetary magnetosphere and can lead to mass loss from the

atmosphere. In order to understand how the atmospheres of planets

evolve, it is necessary to know the properties of these stellar winds.

We study the winds of low-mass stars within the framework of the project

Pathways to Habitability (http://path.univie.ac.at/). We investigate the

winds in both single and binary star systems.

Organisation(en)
Institut für Astrophysik
Externe Organisation(en)
Russian Academy of Sciences
Publikationsdatum
07-2013
ÖFOS 2012
103004 Astrophysik
Link zum Portal
https://ucrisportal.univie.ac.at/de/publications/3bf297f2-2828-435e-b457-f18e9ce38287