Magnetic fields in O-, B- and A-type stars on the main sequence
Maryline Briquet
TL;DR
This review summarizes recent observational and theoretical research on magnetic fields in main-sequence stars of spectral types O, B, and A, focusing on stars with radiative envelopes.
Contribution
It compiles the latest observational data and theoretical explanations regarding magnetic fields in these types of stars, providing a comprehensive overview.
Findings
Recent observations confirm the presence of magnetic fields in O, B, and A-type stars.
Theoretical models are advancing to explain the origin and evolution of these magnetic fields.
The review highlights gaps and future directions in understanding stellar magnetism.
Abstract
In this review, the latest observational results on magnetic fields in main-sequence stars with radiative envelopes are summarised together with the theoretical works aimed at explaining them.
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.