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Understanding Balmer Decrements in T Tauri Stars in Terms of Multiflow Magnetospheric Accretion

Magnetospheric accretion is the paradigm for accretion in classical T Tauri stars (CTTSs). However, the standard, one-flow magnetospheric accretion model fails to replicate important characteristics such as the observed Balmer decrements. We address this limitation by adopting a model with two axisy...

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Bibliografiske detaljer
Principais autores: Naiara Patiño, Nuria Calvet, Gladis Magris, Marbely Micolta, Thanawuth Thanathibodee, Thomas K. Waters, María José Colmenares
Format: Artigo
Sprog:Inglês
Udgivet: IOP Publishing 2026-01-01
Serier:The Astrophysical Journal
Fag:
Online adgang:https://doi.org/10.3847/1538-4357/ae5d2e
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