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Proceedings Paper

Mid-infrared view of cool evolved stars with the Very Large Telescope Interferometer
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Paper Abstract

Two interferometric instruments at ESO's Very Large Telescope Interferometer (VLTI) - MIDI and AMBER operating in the mid-infrared (8-13 μm) and the near-infrared (JHK), respectively - have proven to be very powerful to study the physical properties of the circumstellar material around evolved stars. With the "spectro-interferometric" capability of MIDI and AMBER, we can disentangle spectral and spatial information on the observed object. VLTI observations have confirmed our pictures on the circumstellar environment of cool evolved stars in some cases but brought about entirely unexpected pictures in other cases. Here, we present our recent results obtained with VLTI/MIDI.

Paper Details

Date Published: 28 July 2008
PDF: 6 pages
Proc. SPIE 7013, Optical and Infrared Interferometry, 70134M (28 July 2008); doi: 10.1117/12.788775
Show Author Affiliations
Keiichi Ohnaka, Max-Planck-Institut für Radioastronomie (Germany)
Thomas Driebe, Max-Planck-Institut für Radioastronomie (Germany)
Karl-Heinz Hofmann, Max-Planck-Institut für Radioastronomie (Germany)
Gerd Weigelt, Max-Planck-Institut für Radioastronomie (Germany)
Markus Wittkowski, European Southern Observatory (Germany)


Published in SPIE Proceedings Vol. 7013:
Optical and Infrared Interferometry
Markus Schöller; William C. Danchi; Françoise Delplancke, Editor(s)

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