130 citations · 448 across the 7 of their papers we have counts for
7 papers
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…
Gas modelling in the disc of HD 163296
I. Tilling, P. Woitke, G. Meeus +19
We present detailed model fits to observations of the disc around the Herbig Ae star HD 163296. This well-studied object has an age of ~ 4 Myr, with evidence of a circumstellar dis…
Continuum and line modeling of disks around young stars II. Line diagnostics for GASPS from the DENT grid
I. Kamp, P. Woitke, C. Pinte +5
Aims. We want to understand the chemistry and physics of disks on the basis of a large unbiased and statistically relevant grid of disk models. One of the main goals is to explore…
Gas in Protoplanetary Discs (GASPS) 1. First results
G. S. Mathews, W. R. F. Dent, J. P. Williams +50
Context - Circumstellar discs are ubiquitous around young stars, but rapidly dissipate their gas and dust on timescales of a few Myr. The Herschel space observatory allows for the…
Continuum and line modelling of discs around young stars. I. 300000 disc models for Herschel/GASPS
Peter Woitke, Christophe Pinte, Ian Tilling +5
We have combined the thermo-chemical disc code ProDiMo with the Monte Carlo radiative transfer code MCFOST to calculate a grid of ~300000 circumstellar disc models, systematically…
Radiation thermo-chemical models of protoplanetary disks II. Line diagnostics
I. Kamp, I. Tilling, P. Woitke +2
Methods. We use the recently developed disk code ProDiMo to calculate the physico-chemical structure of protoplanetary disks and apply the Monte-Carlo line radiative transfer code…
Disc evolution and the relationship between and in T Tauri stars
I. Tilling, C. J. Clarke, J. E. Pringle +1
We investigate the evolution of accretion luminosity and stellar luminosity in pre-mainsequence stars. We make the assumption that when the star appears as…