My main area of interest is in protostellar disks dynamics and evolution.
I am using SPH (Smoothed Particle Hydrodynamics)
to model gaseous accretion disks, investigating their instabilities and
evolution. I have worked on instabilities in
massive
protostellar disks, as well as gap formation in protoplanetary and
circumbinary disks. I also have a two-phase
dusty+gas SPH code for building planets which keeps me busy.
To compare models with observations, I make synthetic IR maps.
Papers
A list of papers published, submitted and in
preparation.
Last updated: Thursday, 29-Sep-2011 22:18:06 EST
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