2006/08/25 by P. Leto, C. Trigilio, C. S. Buemi +2 · 1 citation
Physics and Astronomy · #Astro and Planetary Science #Astronomy #Astrophysics #Magnetic field #Magnetosphere #Observable #Physics #Solar and Space Plasma Dynamics #Stars #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1051/0004-6361:20054511
10 pages, 7 figures, A&A in press
openalex publication_date 2006/08/25 · arxiv created 2006/10/13 · arxiv updated 2009/12/01 · openalex created_date 2022/08/20 · openalex updated_date 2026/07/31
Aims.In order to fully understand the physical processes in the magnetospheres of the Magnetic Chemically Peculiar stars, we performed multi-frequency radio observations of CU Virginis. The radio emission of this kind of stars arises from the interaction between energetic electrons and magnetic field. Our analysis is used to test the physical scenario proposed for the radio emission from the MCP stars and to derive quantitative information about physical parameters not directly observable.