Paper
12 September 2012 To be or not to be asymmetric? VLTI and the mass loss geometry of red giants
Claudia Paladini, Daniela Klotz, Stephane Sacuto, Josef Hron, Markus Wittkowski, Eric Lagadec, Tijl Verhoelst, Alain Jorissen, Andrea Richichi, Martin Groenewegen, Hans Olofsson, Franz Kerschbaum
Author Affiliations +
Abstract
The mass-loss process is a key ingredient for our understanding in many fields of astrophysics, including stellar evolution and the enrichment of the interstellar medium (ISM) via stellar yields. We combined the capability of the VLTI/MIDI and VLT/VISIR instruments with very recent Herschel/PACS observations to characterize the geometry of mass loss from evolved red giants on the Asymptotic Giant Branch (AGB) at various scales. This paper describes the sample of objects, the observing strategy, the tool for the interpretation, and preliminary MIDI results for two targets: U Ant and θ Aps.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Claudia Paladini, Daniela Klotz, Stephane Sacuto, Josef Hron, Markus Wittkowski, Eric Lagadec, Tijl Verhoelst, Alain Jorissen, Andrea Richichi, Martin Groenewegen, Hans Olofsson, and Franz Kerschbaum "To be or not to be asymmetric? VLTI and the mass loss geometry of red giants", Proc. SPIE 8445, Optical and Infrared Interferometry III, 84451R (12 September 2012); https://doi.org/10.1117/12.926380
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KEYWORDS
Stars

Atmospheric modeling

Spherical lenses

Visibility

Data modeling

Interferometry

Astronomy

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