Binary-induced magnetic activity?

2011/08/23 by K. G. Strassmeier, T. A. Carroll, M. Weber +5
Physics and Astronomy · #Astro and Planetary Science #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Binary star #Magnetic field #Orbital eccentricity #Orbital motion #Orbital period #Photometry (optics) #Physics #Planet #Rotation period #Spectral line #Stars #Starspot #Stellar rotation #Stellar, planetary, and galactic studies #Zeeman effect #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201117167

published as A&A 535 (2011) A98

arxiv created 2011/08/23 · openalex publication_date 2011/08/29 · arxiv updated 2012/08/21 · openalex created_date 2022/10/01 · openalex updated_date 2026/08/05

Abstract

Context. Multi-wavelength time-series observations with high cadence and long duration are needed to resolve and understand the many variations of magnetically active late-type stars, which is an approach often used to observe the Sun.

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