Publications (17)
Coordinated AMBER and MIDI observations of the Mira variable RR Aql
Iva Karovicova, Markus Wittkowski, David A. Boboltz +1
Parsec-scale dust distributions in Seyfert galaxies - Results of the MIDI AGN snapshot survey
Konrad R. W. Tristram, David Raban, Klaus Meisenheimer +11
Planet Formation Imager (PFI): science vision and key requirements
Stefan Kraus, John D. Monnier, Michael J. Ireland +75
Spatially resolved dusty torus toward the red supergiant WOH G64 in the Large Magellanic Cloud
Keiichi Ohnaka, Thomas Driebe, Karl-Heinz Hofmann +2
From the atmosphere to the circumstellar environment in cool evolved stars
Markus Wittkowski, Claudia Paladini
VLTI status update: a decade of operations and beyond
Antoine Merand, Roberto Abuter, Emmanuel Aller-Carpentier +44
VINCI-VLTI measurements of HR 4049: the physical size of the circumbinary envelope
Simone Antoniucci, Francesco Paresce, Markus Wittkowski
A high-mass protobinary system with spatially resolved circumstellar accretion disks and circumbinary disk
Stefan Kraus, Jacques Kluska, Alexander Kreplin +9
Multiple Star Systems in the Orion Nebula
GRAVITY collaboration, Martina Karl, Oliver Pfuhl +133
Cool, evolved stars: results, challenges, and promises for the next decade
Gioia Rau, Rodolfo Montez, Kenneth G. Carpenter +27
Mass Losing Asymptotic Giant Branch Stars and Supergiants
Patricia A. Whitelock, Martha Boyer, Susanne Höfner +2
Asymmetric silicate dust distribution toward the silicate carbon star BM Gem
Keiichi Ohnaka, Hideyuki Izumiura, Christoph Leinert +3
The potential of near-infrared high-resolution studies on the field of galaxies in the young universe
Markus Wittkowski
Observing the Seyfert 2 nucleus of NGC 1068 with the VLT Interferometer
Huub Rottgering, Walter Jaffe, Klaus Meisenheimer +4
Joint VLTI/VLBA observations of Mira stars
Markus Wittkowski, David A. Boboltz
Science cases for a visible interferometer
Philippe Stee, France Allard, Myriam Benisty +54
Round Table Summary: Stellar interferometry as a tool to investigate atmospheres and to compare observations with models
Markus Wittkowski