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Interferometric view into RT Pav's long secondary period. binary vs oscillatory convective modes

Fuente: arXiv

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Detalles Bibliográficos
Autores principales:	Courtney-Barrer, B., Haubois, X., Wood, P., Dionese, D., Decin, L., Paladini, C., Mellah, I. El, Defrère, D., Ireland, M.
Formato:	Preprint
Publicado:	2025
Materias:	Solar and Stellar Astrophysics
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

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