Theo Chousinho Khouri Silva investigates the mass-loss mechanisms of oxygen-rich asymptotic giant branch (AGB) stars by modelling data that was mainly acquired with the Herschel telescope. He focuses on low-mass-loss rate oxygen-rich sources and pursues comprehensive models in which gaseous and dusty envelopes are modelled together.
T. Chousinho Khouri Silva, Oxygen-Rich AGB Stars with Low Mass-Loss Rate Observed with Herschel.
Prof. A. de Koter
Prof. L.B.F.M. Waters
Prof. L. Decin (KU Leuven)
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