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To be or not to be asymmetric? VLTI and the mass loss geometry of red giants
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- Paladini, C. (author)
- Universität Wien,University of Vienna
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- Klotz, D. (author)
- Universität Wien,University of Vienna
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- Sacuto, S. (author)
- Uppsala universitet,Teoretisk astrofysik,Uppsala University
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- ISBN 9780819491466
- SPIE, 2012
- 2012
- English.
- In: Proceedings of SPIE - The International Society for Optical Engineering. - : SPIE. - 0277-786X .- 1996-756X. - 9780819491466 ; 8445, s. Art. no. 84451R-
- Conference paper (peer-reviewed)
Abstract
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- 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.
Subject headings
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
Keyword
- Herschel
- Imaging
- Stellar atmospheres
- Optical interferometry
- Infrared
- Mass-loss
- Late-type stars
Publication and Content Type
- kon (subject category)
- ref (subject category)
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- Hron, J.
- Wittkowski, M.
- Lagadec, E.
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- Verhoelst, T.
- Jorissen, A.
- Richichi, A.
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- Kerschbaum, F.
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- Chalmers University of Technology
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