activity
20152026
most citedConsistent dust and gas models for protoplanetary disks. I. Disk shape, dust settling, opacities, and PAHs

379 citations · 1.4k across the 35 of their papers we have counts for

collaborators
Showing 2022Show all

5 papers · 1 filter

astro-ph.EP2022★ 8 cited

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…

astro-ph.SR2022★ 18 cited

Interpreting molecular hydrogen and atomic oxygen line emission of T Tauri disks with photoevaporative disk-wind models

Ch. Rab, M. Weber, T. Grassi +6

Winds in protoplanetary disks play an important role in their evolution and dispersal. However, what physical process is driving the winds is still unclear (i.e. magnetically vs th…

astro-ph.SR2022★ 10 cited

Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): Scattered light detection of a possible disk wind in RY Tau

P. -G. Valegård, C. Ginski, C. Dominik +14

Disk winds are an important mechanism for accretion and disk evolution around young stars. The accreting intermediate-mass T-Tauri star RY Tau has an active jet and a previously kn…

astro-ph.EP2022★ 13 cited

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…

astro-ph.EP2022★ 9 cited

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…