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Winds of AGB Stars - The Role of Stellar Pulsation
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Theoretical Astrophysics.
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Theoretical Astrophysics.
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Theoretical Astrophysics.
2015 (English)In: WHY GALAXIES CARE ABOUT AGB STARS III: A CLOSER LOOK IN SPACE AND TIME, ASTRONOMICAL SOC PACIFIC , 2015, Vol. 497, 127-128 p.Conference paper (Refereed)Text
Abstract [en]

Changing the stellar pulsation properties has large impact on the behavior of the atmosphere of C-type AGB stars. This relationship is examined.

Place, publisher, year, edition, pages
ASTRONOMICAL SOC PACIFIC , 2015. Vol. 497, 127-128 p.
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:uu:diva-294833ISI: 000371098100023ISBN: 9781583818794OAI: oai:DiVA.org:uu-294833DiVA: diva2:953816
Conference
Conference on Why Galaxies Care About AGB Stars III: A Closer Look in Space and Time, JUL 28-AUG 01, 2014, Univ Vienna, Vienna, AUSTRIA
Available from: 2016-08-18 Created: 2016-05-27 Last updated: 2016-08-18Bibliographically approved

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Liljegren, SofieHöfner, SusanneEriksson, Kjell
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