Sun-like Stars: Magnetic fields, cycles and exoplanets

Research output: Contribution to journalArticlepeer-review

Abstract

In Sun-like stars, magnetic fields are generated in the outer convective layers. They shape the stellar environment, from the photosphere to planetary orbits. Studying the large-scale magnetic field of those stars enlightens our understanding of the field properties and gives us observational constraints for field generation dynamo models. It also sheds light on how normal the Sun is among Sun-like stars. In this contribution, I will review the field properties of Sun-like stars, focusing on solar twins and planet hosting stars. I will discuss the observed large-scale magnetic cycles, compare them to stellar activity cycles, and link that to what we know about the Sun. I will also discuss the effect of large-scale stellar fields on exoplanets, exoplanetary emissions (e.g. radio), and habitability.

Original languageEnglish
Pages (from-to)360-364
Number of pages5
JournalProceedings of the International Astronomical Union
Volume11
Issue numberA29A
DOIs
Publication statusPublished - 2015
Externally publishedYes

Keywords

  • stars: activity
  • stars: magnetic fields
  • technique: polarimetry

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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