activity
20032017
most citedDiagnostics of irradiated gas in galaxy nuclei. I: A Far-ultraviolet and X-ray dominated region code

421 citations · 6.2k across the 71 of their papers we have counts for

collaborators

70 papers

astro-ph.SR2017★ 38 cited

X-ray radiative transfer in protoplanetary disks - The role of dust and X-ray background fields

Ch. Rab, M. Güdel, P. Woitke +5

The X-ray luminosities of T Tauri stars are about two to four orders of magnitude higher than the luminosity of the contemporary Sun. As these stars are born in clusters, their dis…

astro-ph.GA2017★ 93 cited

Molecular gas in three z~7 quasar host galaxies

Bram Venemans, Fabian Walter, Roberto Decarli +6

We present ALMA band 3 observations of the CO(6-5), CO(7-6), and [CI] 369micron emission lines in three of the highest redshift quasar host galaxies at 6.6<z<6.9. These measurement…

astro-ph.GA2016★ 16 cited

The outflow of gas from the Centaurus A circumnuclear disk: atomic spectral line maps from Herschel-PACS and APEX

F. P. Israel, R. Guesten, R. Meijerink +2

The physical state of the gas in the central 500 pc of NGC~5128 (the radio galaxy Centaurus A - Cen A), was investigated using the far-infrared fine-structure lines of carbon, oxyg…

astro-ph.EP2016★ 10 cited

The mid-IR water and silicate relation in protoplanetary disks

S. Antonellini, J. Bremer, I. Kamp +7

Mid-IR water lines from protoplanetary disks around T Tauri stars have a detection rate of 50\%. Models have identified multiple physical properties of disks such as dust-to-gas ma…

astro-ph.GA2016★ 108 cited

Multi-phase Nature of a Radiation-Driven Fountain with Nuclear Starburst in a Low-mass Active Galactic Nucleus

Keiichi Wada, Marc Schartmann, Rowin Meijerink

The structures and dynamics of molecular, atomic, and ionized gases are studied around a low-luminosity active galactic nucleus (AGN) with a small () black ho…

astro-ph.GA2016★ 25 cited

Surface chemistry in photodissociation regions

G. B. Esplugues, S. Cazaux, R. Meijerink +2

The presence of dust can strongly affect the chemical composition of the interstellar medium. We model the chemistry in photodissociation regions (PDRs) using both gas-phase and du…