João M. A. Vilas Boas
It is widely known that the presence of active regions, created by strong local magnetic phenomena, induces RV variations by different physical processes. In this context, we discuss the effects of active regions in the stellar activity and the possibility of modelling the chromospheric emission.
We present integrated changes in SOAP 2.0 software tool that incorporate simple models of chromospheric activity and we conclude about the importance of this study to push forward our ability to detect exoplanets.
2017 July 12, 14:00
Centro de Astrofísica da Universidade do Porto (Classroom)
Rua das Estrelas, 4150-762 Porto