activity
20182021
most citedParsec-scale Dusty Winds in Active Galactic Nuclei: Evidence for Radiation Pressure Driving

31 citations · 53 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.EP202112 cited

First MATISSE L-band observations of HD 179218. Is the inner 10 au region rich in carbon dust particles?

E. Kokoulina, A. Matter, B. Lopez +58

Carbon is one of the most abundant components in the Universe. While silicates have been the main focus of solid phase studies in protoplanetary discs (PPDs), little is known about…

astro-ph.IM202110 cited

Potential and sky coverage for off-axis fringe tracking in optical long baseline interferometry

Abdelkarim Boskri, Romain G. Petrov, Thami El Halkouj +6

The spectacular results provided by the second-generation VLTI instruments GRAVITY and MATISSE on active galactic nuclei (AGN) trigger and justify a strong increase in the sensitiv…

astro-ph.GA2021

Resolving the Hot Dust Disk of ESO323-G77

James H. Leftley, Konrad R. W. Tristram, Sebastian F. Hönig +3

Infrared interferometry has fuelled a paradigm shift in our understanding of the dusty structure in the central parsecs of Active Galactic Nuclei (AGN). The dust is now thought to…

astro-ph.GA201931 cited

Parsec-scale Dusty Winds in Active Galactic Nuclei: Evidence for Radiation Pressure Driving

James H. Leftley, Sebastian F. Hönig, Daniel Asmus +5

Infrared interferometry of local AGN has revealed a warm (~300K-400K) polar dust structure that cannot be trivially explained by the putative dust torus of the unified model. This…

astro-ph.GA2018

New evidence for the dusty wind model: Polar dust and a hot core in the type-1 Seyfert ESO323-G77

James Leftley, Konrad Tristram, Sebastian Hönig +3

Infrared interferometry of Seyfert galaxies has revealed that their warm (K) dust emission originates primarily from polar regions instead of from an equatorial dust tor…