Observed variations of the global longitudinal magnetic fields of stars
V.D. Bychkov, L.V. Bychkova, J. Madej

TL;DR
This paper reviews observed variations in the longitudinal magnetic fields across 218 stars, highlighting differences among various stellar types including chemically peculiar stars, supergiants, red dwarfs, and planet-hosting stars.
Contribution
It provides a comprehensive overview of magnetic field observations across diverse star types, summarizing current knowledge and identifying patterns in magnetic field variations.
Findings
172 stars are chemically peculiar with measured magnetic phase curves
Magnetic properties vary significantly among different spectral types
The review highlights the diversity of magnetic field behaviors in stars
Abstract
Actually there exist 218 stars with measured phase curves of the longitudinal (effective) magnetic field B_e. 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.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Solar and Space Plasma Dynamics
