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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.

Event details of Oxygen-rich AGB stars with low mass-loss rate
Date 16 December 2014
Time 12:00 -13:00
Location Agnietenkapel

T. Chousinho Khouri Silva, Oxygen-Rich AGB Stars with Low Mass-Loss Rate Observed with Herschel.

Supervisors

Prof. A. de Koter
Prof. L.B.F.M. Waters

Co-supervisor

Prof. L. Decin (KU Leuven)

Agnietenkapel

Oudezijds Voorburgwal 229 - 231
1012 EZ Amsterdam

Entrance

This event is open to the public.