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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 5.

Comparison between the planetary magnetospheric size and the star’s age for the E. N. Parker (1958) model using WTTS data and data from V. See et al. (2014), color coded by chromospheric activity. The figure also includes the Earth’s position, based on the Sun, which has an age of 4.57 Gyr (A. Bonanno et al. 2002).

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