activity
20132026
most citedChemical enrichment of giant planets and discs due to pebble drift

242 citations · 993 across the 58 of their papers we have counts for

collaborators
Showing 2019Show all

5 papers · 1 filter

astro-ph.EP2019

The First Detection of 13C17O in a Protoplanetary Disk: a Robust Tracer of Disk Gas Mass

Alice S. Booth, Catherine Walsh, John D. Ilee +4

Measurements of the gas mass are necessary to determine the planet formation potential of protoplanetary disks. Observations of rare CO isotopologues are typically used to determin…

astro-ph.EP2019

First detections of H13CO+ and HC15N in the disk around HD 97048: Evidence for a cold gas reservoir in the outer disk

Alice S. Booth, Catherine Walsh, John D. Ilee

Observations of different molecular lines in protoplanetary disks provide valuable information on the gas kinematics, as well as constraints on the radial density and temperature s…

astro-ph.EP2019142 cited

Planet-forming material in a protoplanetary disc: the interplay between chemical evolution and pebble drift

Richard A. Booth, John D. Ilee

The composition of gas and solids in protoplanetary discs sets the composition of planets that form out of them. Recent chemical models have shown that the composition of gas and d…

astro-ph.EP2019

Planet formation: The case for large efforts on the computational side

Wladimir Lyra, Thomas Haworth, Bertram Bitsch +54

Modern astronomy has finally been able to observe protoplanetary disks in reasonable resolution and detail, unveiling the processes happening during planet formation. These observe…

astro-ph.SR201932 cited

Consistent dust and gas models for protoplanetary disks IV. A panchromatic view of protoplanetary disks

O. Dionatos, P. Woitke, M. Guedel +17

Consistent modeling of protoplanetary disks requires the simultaneous solution of both continuum and line radiative transfer, heating/cooling balance between dust and gas and, of c…