2008/02/04 by J. D. Landstreet, J. Silaj, V. Andretta +8
Physics and Astronomy · #Astro and Planetary Science #Astrophysics and Star Formation Studies #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1051/0004-6361:20078884
accepted by Astronomy & Astrophysics
openalex publication_date 2008/02/04 · arxiv created 2008/03/06 · arxiv updated 2009/12/01 · openalex created_date 2020/11/23 · openalex updated_date 2026/07/31
Context. A small fraction of upper main sequence stars have strong, highly structured magnetic fields. The origin and evolution of these fields are not adequately understood.