activity
20032008
most citedTechnetium and the third dredge up in AGB stars II. Bulge stars

56 citations · 56 across the 4 of their papers we have counts for

collaborators

9 papers

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-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-ph2008

Milli-arcsecond astrophysics with VSI, the VLTI spectro-imager in the ELT era

F. Malbet, D. Buscher, G. Weigelt +49

Nowadays, compact sources like surfaces of nearby stars, circumstellar environments of stars from early stages to the most evolved ones and surroundings of active galactic nuclei c…

astro-ph200656 cited

Technetium and the third dredge up in AGB stars II. Bulge stars

Stefan Uttenthaler, Josef Hron, Thomas Lebzelter +3

We searched for Technetium (Tc) in a sample of bright oxygen-rich asymptotic giant branch (AGB) stars located in the outer galactic bulge. Tc is an unstable element synthesised via…

astro-ph2005

Atmospheric dynamics in carbon-rich Miras. II. Models meet observations

W. Nowotny, T. Lebzelter, J. Hron +1

Originating in different depths of the very extended atmospheres of AGB stars, various molecular spectral lines observable in the near-infrared show diverse behaviours and can be u…

astro-ph2005

Synthetic Line Profiles for Pulsating Red Giants

W. Nowotny, B. Aringer, S. Hoefner +3

Pulsation influences atmospheric structures of variable AGB stars (Miras) considerably. Spectral lines of the CO dv=3 vibration-rotation bands (at 1.6mue) therefore have a very cha…