The Frequency-independent Radio Luminosity–Orbital/Rotational Period Relation of RS CVn Stars
Radio emissions from RS CVn objects exhibit distinct characteristics at low and high frequencies, widely attributed to differing radiation mechanisms. The disparate processes of high-frequency gyrosynchrotron and low-frequency electron cyclotron maser emissions have traditionally suggested an absenc...
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| Principais autores: | , |
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| 格式: | Artigo |
| 語言: | Inglês |
| 出版: |
IOP Publishing
2025-01-01
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| 叢編: | The Astrophysical Journal |
| 主題: | |
| 在線閱讀: | https://doi.org/10.3847/1538-4357/ae003c |
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