Transition from super-alfvenic to sub-alfvenic stellar wind flow passing by an exoplanet, using the example of HD 209458b
- Authors: Belenkaya E.S.1
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Affiliations:
- Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics (SINP MSU)
- Issue: Vol 101, No 3 (2024)
- Pages: 244-249
- Section: Articles
- URL: https://rjsvd.com/0004-6299/article/view/647617
- DOI: https://doi.org/10.31857/S0004629924030053
- EDN: https://elibrary.ru/KJSTYR
- ID: 647617
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