179 citations · 3k across the 60 of their papers we have counts for
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Small vs large dust grains in transitional disks: do different cavity sizes indicate a planet?
Antonio Garufi, Sascha P Quanz, Henning Avenhaus +7
Transitional disks represent a short stage of the evolution of circumstellar material. Studies of dust grains in these objects can provide pivotal information on the mechanisms of…
Giant Planet Formation, Evolution, and Internal Structure
Ravit Helled, Peter Bodenheimer, Morris Podolak +7
The large number of detected giant exoplanets offers the opportunity to improve our understanding of the formation mechanism, evolution, and interior structure of gas giant planets…
Large grains can grow in circumstellar discs
Farzana Meru, Marina Galvagni, Christoph Olczak +1
We perform coagulation & fragmentation simulations to understand grain growth in T Tauri & brown dwarf discs. We present a physically-motivated approach using a probability distrib…
Growth and fragmentation of centimetre-sized dust aggregates: the dependence on aggregate size and porosity
Farzana Meru, Ralf J. Geretshauser, Christoph Schaefer +2
We carry out three-dimensional Smoothed Particle Hydrodynamics simulations of spherical homogeneous SiO2 dust aggregates to investigate how the mass and the porosity of the aggrega…
Growth of grains in Brown Dwarf disks
Farzana Meru, Marina Galvagni, Christoph Olczak
We perform coagulation and fragmentation simulations using the new physically-motivated model by Garaud et al. (2013) to determine growth locally in brown dwarf disks. We show that…
Triggered fragmentation in gravitationally unstable discs: forming fragments at small radii
Farzana Meru
We carry out three dimensional radiation hydrodynamical simulations of gravitationally unstable discs using to explore the movement of mass in a disc following its fragmentation. C…