activity
20102024
most citedConsistent dust and gas models for protoplanetary disks. I. Disk shape, dust settling, opacities, and PAHs

379 citations · 1.3k across the 27 of their papers we have counts for

collaborators
Showing 2013Show all

6 papers · 1 filter

astro-ph.GA2013

Gas signatures of Herbig Ae/Be disks probed with Herschel SPIRE spectroscopy

Matthijs H. D. van der Wiel, David A. Naylor, Giambattista Aresu +1

Herbig Ae/Be objects, like their lower mass counterparts T Tauri stars, are seen to form a stable circumstellar disk which is initially gas-rich and could ultimately form a planeta…

astro-ph.GA2013★ 51 cited

Gas lines from the 5-Myr old optically thin disk around HD141569A. Herschel observations and modeling

Wing-Fai Thi, Christophe Pinte, Eric Pantin +20

At the distance of 99-116 pc, HD141569A is one of the nearest HerbigAe stars that is surrounded by a tenuous disk, probably in transition between a massive primordial disk and a de…

astro-ph.SR2013★ 63 cited

Uncertainties in water chemistry in disks: An application to TW Hya

I. Kamp, W. -F. Thi, G. Meeus +7

Context. This paper discusses the sensitivity of water lines to chemical processes and radiative transfer for the protoplanetary disk around TW Hya. The study focuses on the Hersch…

astro-ph.GA2013★ 18 cited

Tracing the Physical Conditions in Active Galactic Nuclei with Time-Dependent Chemistry

Rowin Meijerink, Marco Spaans, Inga Kamp +3

We present an extension of the code ProDiMo that allows for a modeling of processes pertinent to active galactic nuclei and to an ambient chemistry that is time dependent. We prese…

astro-ph.GA2013★ 128 cited

GASPS - a Herschel survey of gas and dust in Protoplanetary Disks: Summary and Initial Statistics

W. R. F. Dent, W. F. Thi, I. Kamp +47

GASPS is a far-infrared line and continuum survey of protoplanetary and young debris disks using PACS on the Herschel Space Observatory. The survey includes [OI] at 63 microns, as…

astro-ph.SR2013★ 91 cited

Water vapor in the protoplanetary disk of DG Tau

L. Podio, I. Kamp, C. Codella +13

Water is key in the evolution of protoplanetary disks and the formation of comets and icy/water planets. While high excitation water lines originating in the hot inner disk have be…