197 citations · 1k across the 28 of their papers we have counts for
28 papers
Laboratory experiments on the sublimation of methane through ice dust layers and applications to cometary activity
Carla Tamai, Belen Mate, Stephanie Cazaux +1
Context. Comets are small celestial bodies made of ice, dust, and rock that orbit the Sun. Understanding their behavior as they warm up at perihelion unveils many pieces of informa…
Circumplanetary disk ices II. Composition
Nickolas Oberg, Stephanie Cazaux, Inga Kamp +3
The subsurface oceans of icy satellites are among the most compelling among the potentially habitable environments in our Solar System. The question of whether a liquid subsurface…
Observing Circumplanetary Disks with METIS
Nickolas Oberg, Inga Kamp, Stephanie Cazaux +2
Context: A full understanding of the planet and moon formation process requires observations that probe the circumplanetary environment of accreting giant planets. The mid-infrared…
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…
Circumplanetary disk ices. I. Ice formation vs. viscous evolution and grain drift
Nickolas Oberg, Inga Kamp, Stephanie Cazaux +2
The large icy moons of Jupiter formed in a circumplanetary disk (CPD). CPDs are fed by infalling circumstellar gas and dust which may be shock-heated upon accretion or sublimated w…
Thermal desorption of interstellar ices. A review on the controlling parameters and their implications fromsnowlines to chemical complexity
Marco Minissale, Yuri Aikawa, Edwin Bergin +16
The evolution of star-forming regions and their thermal balance are strongly influenced by their chemical composition, that, in turn, is determined by the physico-chemical processe…