Should we observe spirals in young planet-forming discs?
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We live in exciting times where new observations are hinting to us that planets may form early on in planet-forming discs. Young discs are expected to exhibit spiral structures, yet only few observations actually show spirals that are indicative of young discs. In this colloquium I will explore some of the possible reasons why this might be, and in particular I will look at processes that occur in discs which might act to erase the spiral structures.
This talk is part of the Institute of Astronomy Colloquia series.
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