papers

Publications (13)

astro-ph.SR2017

Gas dynamics in the inner few AU around the Herbig B[e] star MWC297: Indications of a disk wind from kinematic modeling and velocity-resolved interferometric imaging

Edward Hone, Stefan Kraus, Alexander Kreplin +4

We present near-infrared AMBER (R = 12, 000) and CRIRES (R = 100, 000) observations of the Herbig B[e] star MWC297 in the hydrogen Br-gamma-line. Using the VLTI unit telescopes, we…

astro-ph.SR2019

The TORUS radiation transfer code

Tim Harries, Tom Haworth, David Acreman +2

We present a review of the TORUS radiation transfer and hydrodynamics code. TORUS uses a 1-D, 2-D or3-D adaptive mesh refinement scheme to store and manipulate the state variables,…

astro-ph2008

Phase Referencing in Optical Interferometry

Mercedes E. Filho, Paulo Garcia, Gilles Duvert +20

One of the aims of next generation optical interferometric instrumentation is to be able to make use of information contained in the visibility phase to construct high dynamic rang…

astro-ph2004

Linear spectropolarimetry of young and other emission line stars

Janet Drew, Jorick Vink, Tim Harries +2

The aim of this article is to demonstrate the useful role that can be played by spectropolarimetric observations of young and evolved emission line stars that analyse the linearly…

astro-ph.EP2022

Gemini-LIGHTS: Herbig Ae/Be and massive T-Tauri protoplanetary disks imaged with Gemini Planet Imager

Evan A. Rich, John D. Monnier, Alicia Aarnio +20

We present the complete sample of protoplanetary disks from the Gemini- Large Imaging with GPI Herbig/T-tauri Survey (Gemini-LIGHTS) which observed bright Herbig Ae/Be stars and T-…

astro-ph.IM2014

The Science Case for the Planet Formation Imager (PFI)

Stefan Kraus, John Monnier, Tim Harries +16

Among the most fascinating and hotly-debated areas in contemporary astrophysics are the means by which planetary systems are assembled from the large rotating disks of gas and dust…

astro-ph2005

VITRUV - Science Cases

Paulo J. V. Garcia, Jean-Phillipe Berger, Romano Corradi +11

VITRUV is a second generation spectro-imager for the PRIMA enabled Very Large Telescope Interferometer. By combining simultaneously up to 8 telescopes VITRUV makes the VLTI up to 6…

astro-ph.SR2010

On the properties of discs around accreting brown dwarfs

Nathan Mayne, Tim Harries

We present a grid of models of accreting brown dwarf systems with circumstellar discs. The calculations involve a self-consistent solution of both vertical hydrostatic and radiativ…

astro-ph.SR2016

TYC 8241 2652 1 and the case of the disappearing disk: no smoking gun yet

Hans Moritz Günther, Stefan Kraus, Carl Melis +12

TYC 8241 2652 1 is a young star that showed a strong mid-infrared (mid-IR, 8-25 mu) excess in all observations before 2008 consistent with a dusty disk. Between 2008 and 2010 the m…

astro-ph.SR2017

High-cadence, High-resolution Spectroscopic Observations of Herbig Stars HD 98922 and V1295 Aquila

Alicia Aarnio, John Monnier, Tim Harries +4

Recent observational work has indicated that mechanisms for accretion and outflow in Herbig Ae/Be star-disk systems may differ from magnetospheric accretion (MA) as it is thought t…

astro-ph2008

Phase Closure Image Reconstruction for Future VLTI Instrumentation

Mercedes E. Filho, Stephanie Renard, Paulo Garcia +21

Classically, optical and near-infrared interferometry have relied on closure phase techniques to produce images. Such techniques allow us to achieve modest dynamic ranges. In order…

astro-ph.EP2018

Is the spiral morphology of the Elias 2-27 circumstellar disc due to gravitational instability?

Cassandra Hall, Ken Rice, Giovanni Dipierro +3

A recent ALMA observation of the Elias 2-27 system revealed a two-armed structure extending out to ~300 au in radius. The protostellar disc surrounding the central star is unusuall…

astro-ph.SR2018

A multi-instrument and multi-wavelength high angular resolution study of MWC614: quantum heated particles inside the disk cavity

Jacques Kluska, Stefan Kraus, Claire L. Davies +13

High angular resolution observations of young stellar objects are required to study the inner astronomical units of protoplanetary disks in which the majority of planets form. As t…