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Johan Olofsson MPIA Heidelberg

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The transition disk around TCha<br />

‣ Fact: the disk is dissipating. Question: how <br />

‣ (hint: there is a strong near-IR excess)<br />

‣ Circumbinary disk Single star (optical spectroscopy)<br />

‣ Grain growth Would affect the innermost regions first<br />

‣ Photo-evaporation Same as above<br />

‣ Gap opened by a planet <br />

‣ We need spatially resolved observations !

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