activity
20042008
most citedLow temperature Rosseland opacities with varied abundances of carbon and nitrogen

80 citations · 118 across the 6 of their papers we have counts for

collaborators

9 papers

astro-ph200880 cited

Low temperature Rosseland opacities with varied abundances of carbon and nitrogen

Michael T. Lederer, Bernhard Aringer

We attempt to produce low temperature opacity data incorporating the effects of varied abundances of the elements carbon and nitrogen. For our temperature range of interest, molecu…

astro-ph20087 cited

VSI: the VLTI spectro-imager

F. Malbet, D. Buscher, G. Weigelt +51

The VLTI Spectro Imager (VSI) was proposed as a second-generation instrument of the Very Large Telescope Interferometer providing the ESO community with spectrally-resolved, near-i…

astro-ph200821 cited

The fluorine abundance in a Galactic Bulge AGB star measured from CRIRES spectra

Stefan Uttenthaler, Thomas Lebzelter, Bernhard Aringer +3

We present measurements of the fluorine abundance in a Galactic Bulge Asymptotic Giant Branch (AGB) star. The measurements were performed using high resolution K-band spectra obtai…

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-ph20071 cited

Low temperature mean opacities for the carbon-rich regime

Michael T. Lederer, Bernhard Aringer

Asymptotic Giant Branch (AGB) stars undergo a change in their chemical composition during their evolution. This in turn leads to an alteration of the radiative opacities, especiall…

astro-ph20069 cited

Near-IR spectroscopy of OH/IR stars in the Galactic Centre

E. Vanhollebeke, J. A. D. L. Blommaert, M. Schultheis +2

Context. Galactic Centre (GC) OH/IR stars can be, based on the expansion velocities of their circumstellar shells, divided into two groups which are kinematically different and the…