524 citations · 3.1k across the 56 of their papers we have counts for
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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…
Observed sizes of planet-forming disks trace viscous evolution
L. Trapman, G. Rosotti, A. D. Bosman +2
The evolution of protoplanetary disks is dominated by the conservation of angular momentum, where the accretion of material onto the central star is driven by viscous expansion of…
Missing water in Class I protostellar disks
Daniel Harsono, Magnus Persson, Alyssa Ramos +10
Water is a key volatile that provides insights into the initial stages of planet formation. The low water abundances inferred from water observations toward low-mass protostellar o…
Excess C/H in Protoplanetary Disk Gas from Icy Pebble Drift across the CO Snowline
Ke Zhang, Arthur D. Bosman, Edwin A. Bergin
The atmospheric composition of giant planets carries the information of their formation history. Superstellar C/H ratios are seen in atmospheres of Jupiter, Saturn, and various gia…