Are the surface abundance structures stable in rapidly rotating Ap star 56 Ari?

Fuente: arXiv

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Bibliographic Details
Main Authors:	Potravnov, I., Piskunov, N., Ryabchikova, T.
Format:	Preprint
Published:	2024
Subjects:	Solar and Stellar Astrophysics
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2407.13645