Stellar coronal mass ejections – II. Constraints from spectroscopic observations

ABSTRACT Detections of stellar coronal mass ejections (CMEs) are still rare. Observations of strong Balmer line asymmetries during flare events have been interpreted as being caused by CMEs. Here, we aim to estimate the maximum possible Balmer line fluxes expected from CMEs to infer their detectabil...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2020-05, Vol.494 (3), p.3766-3783
Hauptverfasser:	Odert, P, Leitzinger, M, Guenther, E W, Heinzel, P
Format:	Artikel
Sprache:	eng
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