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

Fuente: arXiv

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Bibliographic Details
Main Authors:	Courtney-Barrer, B., Haubois, X., Wood, P., Dionese, D., Decin, L., Paladini, C., Mellah, I. El, Defrère, D., Ireland, M.
Format:	Preprint
Published:	2025
Subjects:	Solar and Stellar Astrophysics
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2511.21987