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Observed variations of the global longitudinal magnetic fields of stars

2013/07/11 by В. Д. Бычков, V. D. Bychkov, L. V. Bychkova +5
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #FOS: Physical sciences #K-type main-sequence star #Magnetic field #Physics #Planet #Solar and Space Plasma Dynamics #Solar and Stellar Astrophysics (astro-ph.SR) #Stars #Stellar classification #Stellar, planetary, and galactic studies #Supergiant #T Tauri star #astro-ph.SR

paper · pdf · doi:10.48550/arxiv.1307.3124

published in arXiv (Cornell University) (Cornell University) · Putting A Stars into Context (Moscow, June 2013): Proceedings, in print

arxiv created 2013/07/11 · openalex publication_date 2013/07/11 · arxiv updated 2013/07/12 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/06

Abstract

Actually there exist 218 stars with measured phase curves of the longitudinal (effective) magnetic field Be. In that group 172 objects are classified as magnetic chemically peculiar stars (mCP). Remaining objects are stars of various spectral types, from the most massive hot Of? supergiants to low mass red dwarfs and stars with planets. This paper aims to review briefly properties of the observed magnetic field in various types of stars.

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