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- W4300485648 abstract "Strong, stable, and organised magnetic fields are present at the surfaces of a small fraction of OBA stars. These fossil fields exhibit uniform characteristics in stars over a tremendous range of stellar mass, age, temperature, and rotation rate. In hot O- and B-type stars, these magnetic fields couple efficiently to the stellar radiatively driven winds, strongly influencing stellar mass loss and rotation. In this article we review the characteristics of the known magnetic hot stars, discuss recent discoveries and insights, and describe recent theoretical progress toward understanding basic field properties and the influence of magnetic fields on hot star evolution." @default.
- W4300485648 created "2022-10-03" @default.
- W4300485648 creator A5059426403 @default.
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- W4300485648 date "2017-12-27" @default.
- W4300485648 modified "2023-09-26" @default.
- W4300485648 title "Magnetism of hot stars" @default.
- W4300485648 doi "https://doi.org/10.48550/arxiv.1712.09747" @default.
- W4300485648 hasPublicationYear "2017" @default.
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