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