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19982026
most citedRadiation thermo-chemical models of protoplanetary disks I. Hydrostatic disk structure and inner rim

398 citations · 6.9k across the 193 of their papers we have counts for

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Showing 2019Show all

9 papers · 1 filter

astro-ph.EP2019★ 17 cited

The infrared line-emitting regions of T Tauri protoplanetary disks

A. J. Greenwood, I. Kamp, L. B. F. M. Waters +2

Mid-infrared molecular line emission detected with the Spitzer Space Telescope is often interpreted using slab models. However, we need to understand the mid-infrared line emission…

astro-ph.SR2019★ 5 cited

The role of atom tunneling in gas-phase reactions in planet-forming disks

Jan Meisner, Inga Kamp, Wing-Fai Thi +1

This paper investigates the impact of the increased reaction rate constant due to tunneling effects on planet-forming disks. Our aim is to quantify the astrophysical implications o…

astro-ph.EP2019★ 34 cited

The surprisingly low carbon mass in the debris disk around HD 32297

Gianni Cataldi, Yanqin Wu, Alexis Brandeker +18

Gas has been detected in a number of debris disks. It is likely secondary, i.e. produced by colliding solids. Here, we report ALMA Band 8 observations of neutral carbon in the CO-r…

astro-ph.EP2019★ 23 cited

The effects of dust evolution on disks in the mid-IR

A. J. Greenwood, I. Kamp, L. B. F. M. Waters +2

In this paper, we couple together the dust evolution code two-pop-py with the thermochemical disk modelling code ProDiMo. We create a series of thermochemical disk models that simu…

astro-ph.SR2019★ 19 cited

Observing the gas component of circumplanetary disks around wide-orbit planet-mass companions in the (sub)mm regime

Ch. Rab, I. Kamp, C. Ginski +6

Several detections of wide-orbit planet-mass/sub-stellar companions around young solar-like stars were reported in the last decade. The origin of those possible planets is still un…

astro-ph.SR2019★ 32 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…