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On stellar hotspots due to star-planet magnetic interactions: How much power can actually be transmitted to the chromosphere?

Fuente: arXiv

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Detalles Bibliográficos
Autores principales:	Paul, Arghyadeep, Strugarek, Antoine, Réville, Victor
Formato:	Preprint
Publicado:	2025
Materias:	Solar and Stellar Astrophysics Earth and Planetary Astrophysics
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

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