2006/10/17 by C. Catala, E. Alecian, E. Alécian +12 · 4 citations
Physics and Astronomy · #Angular momentum #Astro and Planetary Science #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Biology #Classical mechanics #Context (archaeology) #Genetics #Herbig Ae/Be star #K-type main-sequence star #Magnetic field #Main sequence #Physics #Sequence (biology) #Star (game theory) #Stars #Stellar, planetary, and galactic studies #T Tauri star #astro-ph
paper · pdf · doi:10.1051/0004-6361:20066264
10 pages, 6 figures. accepted by Astronomy & Astrophysics
arxiv created 2006/10/17 · openalex publication_date 2006/11/02 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Context.The general context of this paper is the study of magnetic fields in the pre-main sequence intermediate mass Herbig Ae/Be stars. Magnetic fields are likely to play an important role in pre-main sequence evolution at these masses, in particular in controlling the gains and losses of stellar angular momentum.