Forward modeling solar spectra onto Doppler images of λ And
Context. Due to their high chromospheric activity and photometric variability, RS CVn-type binaries are ideal laboratories for studying stellar surface structures and the corresponding stellar activity relations. However, the atmospheric nature of their primary evolved components (luminosity classes...
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| Principais autores: | , |
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| 格式: | Artigo |
| 語言: | Inglês |
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EDP Sciences
2026-06-01
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| 叢編: | Astronomy & Astrophysics |
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| 在線閱讀: | https://www.aanda.org/articles/aa/full_html/2026/06/aa59430-26/aa59430-26.html |
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