Slingshot prominences: coronal structure, mass loss and spin down

The structure of a star’s coronal magnetic field is a fundamental property that governs the high-energy emission from the hot coronal gas and the loss of mass and angular momentum in the stellar wind. It is, however, extremely difficult to measure. We report a new method to trace this structure in r...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2020-01
Hauptverfasser:	Jardine, M, Cameron, A Collier, Donati, J-F, Hussain, G A J
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Sciences of the Universe Solar and Stellar Astrophysics
Online-Zugang:	Volltext
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