Detection of Stellar Mass Ejections through Extreme Ultraviolet Spectral Lines

Coronal mass ejections (CMEs), since their first observation in 1971, have been widely acknowledged as the most significant eruptive phenomena and the primary cause of catastrophic space weather events within our solar system. Whether similar processes involving stellar mass ejections (SMEs) occur o...

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Hlavní autoři:	Zhixun Cheng, Anchuan Song, Guiping Zhou, Yuming Wang, Hui Tian, Xiaolei Li, Jifeng Liu, Jingxiu Wang
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	IOP Publishing 2026-01-01
Edice:	The Astrophysical Journal
Témata:	Stellar coronal mass ejections Solar coronal mass ejections Solar flares Solar extreme ultraviolet emission Doppler shift Stellar spectral lines
On-line přístup:	https://doi.org/10.3847/1538-4357/ae29a9
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