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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| Glavni autori: | , , , , , , , |
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| Format: | Artigo |
| Jezik: | Inglês |
| Izdano: |
IOP Publishing
2026-01-01
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| Serija: | The Astrophysical Journal |
| Teme: | |
| Online pristup: | https://doi.org/10.3847/1538-4357/ae29a9 |
| Oznake: |
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