Is It Possible to Detect Coronal Mass Ejections on Solar-type Stars through Extreme-ultraviolet Spectral Observations?
Stellar coronal mass ejections (CMEs) from host stars are an important factor that affects the habitability of exoplanets. Although their solar counterparts have been well observed for decades, it is still very difficult to find solid evidence of stellar CMEs. Using the spectral line profile asymmet...
| Những tác giả chính: | , , , , , |
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| Định dạng: | Bài viết |
| Ngôn ngữ: | English |
| Được phát hành: |
IOP Publishing
2024-01-01
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| Loạt: | The Astrophysical Journal |
| Những chủ đề: | |
| Truy cập trực tuyến: | https://doi.org/10.3847/1538-4357/ad2a44 |