47 citations · 133 across the 14 of their papers we have counts for
5 papers
Observability of Photoevaporation Signatures in the Dust Continuum Emission of Transition Discs
Giovanni Picogna, Carolina Schäfer, Barbara Ercolano +3
Photoevaporative disc winds play a key role in our understanding of circumstellar disc evolution, especially in the final stages, and they might affect the planet formation process…
Ices in planet-forming disks: Self-consistent ice opacities in disk models
Aditya M. Arabhavi, Peter Woitke, Stephanie M. Cazaux +3
In cold and shielded environments, molecules freeze out on dust grain surfaces to form ices such as H2O, CO, CO2, CH4, CH3OH, and NH3. In protoplanetary disks, the exact radial and…
The effect of metallicity on the abundances of molecules in protoplanetary disks
R. Guadarrama, Eduard I. Vorobyov, Christian Rab +1
We study the influence of different metallicities on the physical, thermal, and chemical properties of protoplanetary disks, and in particular on the formation and destruction of c…
Dust entrainment in photoevaporative winds: Synthetic observations of transition disks
R. Franz, G. Picogna, B. Ercolano +4
X-ray- and extreme-ultraviolet- (XEUV-) driven photoevaporative winds acting on protoplanetary disks around young T-Tauri stars may strongly impact disk evolution, affecting both g…
The gas disk: Evolution and chemistry
Ch. Rab, C. Baldovin-Saavedra, O. Dionatos +2
Protoplanetary disks are the birthplaces of planetary systems. The evolution of the star-disk system and the disk chemical composition determines the initial conditions for planet…