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
Context . Recent observations of the object UX Tau A containing a pre-transitional disk suggest that the inner disk is misaligned and precessing with respect to the outer disk. These motions lead to a highly dynamic environment that changes the reservoir of dust feeding the star. One of the effects...
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Published in | Astronomy and astrophysics (Berlin) Vol. 696; p. A46 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
01.04.2025
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Online Access | Get full text |
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