papers

Publications (20)

astro-ph2004

The VSOP 5 GHz AGN Survey: III. Imaging Results for the First 102 Sources

W. K. Scott, E. B. Fomalont, S. Horiuchi +17

The VSOP mission is a Japanese-led project to study radio sources with sub-milliarcsec resolution using an orbiting 8 m telescope, HALCA, along with global arrays of Earth-based te…

astro-ph.EP2013

Multiwavelength interferometric observations and modeling of circumstellar disks

A. A. Schegerer, T. Ratzka, P. A. Schuller +3

We investigate the structure of the innermost region of three circumstellar disks around pre-main sequence stars HD 142666, AS 205 N, and AS 205 S. We determine the inner radii of…

astro-ph2006

First AU-scale observations of V1647 Ori with VLTI/MIDI

P. Abraham, L. Mosoni, Th. Henning +4

The young eruptive star V1647 Ori was observed with MIDI, the mid-infrared interferometric instrument at the Very Large Telescope Interferometer (VLTI), on March 2, 2005. We presen…

astro-ph.SR2021

Mid-infrared circumstellar emission of the long-period Cepheid l Carinae resolved with VLTI/MATISSE

V. Hocdé, N. Nardetto, A. Matter +149

The nature of circumstellar envelopes (CSE) around Cepheids is still a matter of debate. The physical origin of their infrared (IR) excess could be either a shell of ionized gas, o…

astro-ph.SR2017

Mid-infrared interferometric variability of DG Tau: implications for the inner-disk structure

J. Varga, K. É. Gabányi, P. Ábrahám +12

Context. DG Tau is a low-mass pre-main sequence star, whose strongly accreting protoplanetary disk exhibits a so-far enigmatic behavior: its mid-infrared thermal emission is strong…

astro-ph.SR2010

Fundamental Vibrational Transition of CO during the Outburst of EX Lupi in 2008

M. Goto, Zs. Regály, C. P. Dullemond +16

We report monitoring observations of the T Tauri star EX Lupi during its outburst in 2008 in the CO fundamental band at 4.6-5.0 um. The observations were carried out at the VLT and…

astro-ph.SR2021

The extended atmosphere and circumstellar environment of the cool evolved star VX Sagittarii as seen by MATISSE

A. Chiavassa, K. Kravchenko, M. Montargès +50

Context. VX Sgr is a cool, evolved, and luminous red star whose stellar parameters are difficult to determine, which affects its classification. Aims. We aim to spatially resolve t…

astro-ph2005

Deep Extragalactic VLBI-Optical Survey (DEVOS): I. Pilot MERLIN and VLBI observations

L. Mosoni, S. Frey, L. I. Gurvits +3

We present the results of the pilot observations of the Deep Extragalactic VLBI-Optical Survey (DEVOS). Our ultimate aim is to collect information on compact structures in a large…

astro-ph.SR2020

The asymmetric inner disk of the Herbig Ae star HD 163296 in the eyes of VLTI/MATISSE: evidence for a vortex?

J. Varga, M. Hogerheijde, R. van Boekel +133

Context. The inner few au region of planet-forming disks is a complex environment. High angular resolution observations have a key role in understanding the disk structure and the…

astro-ph.SR2013

Probing the temporal and spatial variations of dust emission in the protoplanetary disk of DG Tau with VLTI/MIDI - Preliminary results

K. E. Gabanyi, L. Mosoni, A. Juhasz +5

The signatures of dust processing and grain growth - related to the formation of rocky planets - are easily seen in mid-infrared spectral features. One important diagnostic tool in…

astro-ph.SR2009

Episodic formation of cometary material in the outburst of a solar-like young star

P. Ábrahám, A. Juhász, C. P. Dullemond +8

Our Solar System originated in interstellar gas and dust; the latter is in the form of amorphous silicate particles and carbonaceous dust. The composition of cometary material show…

astro-ph.IM2022

MATISSE, the VLTI mid-infrared imaging spectro-interferometer

B. Lopez, S. Lagarde, R. G. Petrov +150

Context:Optical interferometry is at a key development stage. ESO's VLTI has established a stable, robust infrastructure for long-baseline interferometry for general astronomical o…

astro-ph2003

Radio structure of the most distant radio-detected quasar at the ten milli- arcsecond scale

S. Frey, L. Mosoni, Z. Paragi +1

We present a high resolution radio image of SDSS 0836+0054 identified recently as the most distant radio-detected quasar at a redshift of z=5.82. The observation was carried out wi…

astro-ph.SR2009

Interferometric Observations of the Hierarchical Triple System Algol

Sz. Csizmadia, T. Borkovits, Zs. Paragi +10

Algol is a triple stellar system consisting of a close semidetached binary orbited by a third object. Due to the disputed spatial orientation of the close pair, the third body pert…

astro-ph2004

The highest redshift radio quasar as seen with the EVN and the VLA

S. Frey, Z. Paragi, L. Mosoni +1

We report on European VLBI Network (EVN) and Very Large Array (VLA) observations of SDSS J0836+0054, the most distant radio-loud quasar known at present z=5.774). The source, with…

astro-ph2007

The VSOP 5 GHz Active Galactic Nucleus Survey: V. Imaging Results for the Remaining 140 sources

R. Dodson, E. B. Fomalont, K. Wiik +21

In February 1997, the Japanese radio astronomy satellite HALCA was launched to provide the space-bourne element for the VLBI Space Observatory Programme (VSOP) mission. Approximate…

astro-ph.SR2018

VLTI/MIDI atlas of disks around low- and intermediate-mass young stellar objects

J. Varga, P. Ábrahám, L. Chen +13

Context. Protoplanetary disks show large diversity regarding their morphology and dust composition. With mid-infrared interferometry the thermal emission of disks can be spatially…

astro-ph2007

Deep Extragalactic VLBI-Optical Survey (DEVOS) II. Efficient VLBI detection of SDSS quasars

S. Frey, L. I. Gurvits, Z. Paragi +3

Context: The Deep Extragalactic VLBI-Optical Survey (DEVOS) aims at constructing a large sample of compact radio sources up to two orders of magnitude fainter than those studied in…

astro-ph2005

High-resolution radio imaging of the most distant radio quasar SDSS J0836+0054

S. Frey, Z. Paragi, L. Mosoni +1

We observed SDSS J0836+0054, the most distant radio-loud quasar known at present (z=5.774) with the European Very Long Baseline Interferometry (VLBI) Network at the 5 GHz frequency…

astro-ph.SR2013

Dynamics during outburst: VLTI observations of the young eruptive star V1647 Ori during its 2003-2006 outburst

L. Mosoni, N. Sipos, P. Abraham +11

Context: It is hypothesized that low-mass young stellar objects undergo eruptive phases during their early evolution. The outburst of V1647 Ori between 2003 and 2006 offered a rare…