A dusty magnetospheric stream as the physical mechanism responsible for stellar occultations: Interpretation of the TESS light curve of the pre-transitional disk system UX Tau A

Open Access

Fig. 1

Light curve from TESS during Sector 70 and the first part of Sector 71 as in Espaillat et al. (2024). The high-amplitude dips at JD 60 2240 and JD 60 2244 are clearly seen.

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