142 citations · 526 across the 9 of their papers we have counts for
15 papers
Exploring HNC and HCN line emission as probes of the protoplanetary disk temperature
Feng Long, Arthur D. Bosman, Paolo Cazzoletti +6
The distributions and abundances of molecules in protoplanetary disks are powerful tracers of the physical and chemical disk structures. The abundance ratios of HCN and its isomer…
Destruction of refractory carbon grains drives the final stage of proto-planetary disk chemistry
Arthur D. Bosman, Felipe Alarcon, Ke Zhang +1
Here we aim to explore the origin of the strong C2H lines to reimagine the chemistry of protoplanetary disks. There are a few key aspects that drive our analysis. First, C2H is det…
Observing Carbon & Oxygen Carriers in Protoplanetary Disks at Mid-infrared Wavelengths
D. E. Anderson, G. A. Blake, L. I. Cleeves +5
Infrared observations probe the warm gas in the inner regions of planet-forming disks around young sun-like, T Tauri stars. In these systems, HO, OH, CO, CO, CH, an…
Hints for icy pebble migration feeding an oxygen-rich chemistry in the inner planet-forming region of disks
Andrea Banzatti, Ilaria Pascucci, Arthur D. Bosman +9
We present a synergic study of protoplanetary disks to investigate links between inner disk gas molecules and the large-scale migration of solid pebbles. The sample includes 63 dis…
Temperature structures of embedded disks: young disks in Taurus are warm
Merel L. R. van 't Hoff, Daniel Harsono, John J. Tobin +6
The chemical composition of gas and ice in disks around young stars set the bulk composition of planets. In contrast to protoplanetary disks (Class II), young disks that are still…
CO Depletion in Protoplanetary Disks: A Unified Picture Combining Physical Sequestration and Chemical Processing
Sebastiaan Krijt, Arthur D. Bosman, Ke Zhang +3
The gas-phase CO abundance (relative to hydrogen) in protoplanetary disks decreases by up to 2 orders of magnitude from its ISM value , even after accounting for fre…