activity
20032023
most citedDust and Gas in the disc of HL Tauri: Surface density, dust settling, and dust-to-gas ratio

440 citations · 4.8k across the 51 of their papers we have counts for

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Showing 2013Show all

7 papers · 1 filter

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.GA2013★ 79 cited

Herschel/PACS Survey of protoplanetary disks in Taurus/Auriga -- Observations of [OI] and [CII], and far infrared continuum

Christian D. Howard, Göran Sandell, William D. Vacca +17

The Herschel Space Observatory was used to observe ~ 120 pre-main-sequence stars in Taurus as part of the GASPS Open Time Key project. PACS was used to measure the continuum as wel…

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.SR2013★ 45 cited

Gas and dust in the TW Hydrae Association as seen by the Herschel Space Observatory

P. Riviere-Marichalar, C. Pinte, D. Barrado +15

Context. Circumstellar discs are the places where planets form, therefore knowledge of their evolution is crucial for our understanding of planet formation. The Herschel Space Obse…

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.GA2013★ 386 cited

Observations of gas flows inside a protoplanetary gap

Simon Casassus, Gerrit van der Plas, Sebastian Perez M. +16

Gaseous giant planet formation is thought to occur in the first few million years following stellar birth. Models predict that giant planet formation carves a deep gap in the dust…