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Interaction between Winds from Weak-lined T Tauri Stars with Exoplanetary Magnetospheres

  • Authors: Yasmmin F. Tamburus, Natália F. S. Andrade, Guilherme R. C. Sampaio, Vera Jatenco-Pereira

Yasmmin F. Tamburus et al 2026 The Astrophysical Journal 1001 .

  • Provider: AAS Journals

Caption: Figure 6.

Upper panel: Ca II H and K line luminosities vs. bolometric luminosity, color coded by planetary magnetosphere size for the E. N. Parker (1958) model. Lower panel: chromospheric activity as a function of stellar mass, where the dashed line represents the fully convective limit of 0.35 M⊙. Both panels consider WTTS data and solar-type stars from V. See et al. (2014).

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