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Detailed Modelling of the Circumstellar Envelope of the S-type AGB Star W Aquilae
Chalmers, Onsala Space Observ, Gothenburg, Sweden..
Chalmers, Onsala Space Observ, Gothenburg, Sweden..
Chalmers, Onsala Space Observ, Gothenburg, Sweden..
Katholieke Univ Leuven, Inst Sterrenkunde, Louvain, Belgium..
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2015 (English)In: WHY GALAXIES CARE ABOUT AGB STARS III: A CLOSER LOOK IN SPACE AND TIME, ASTRONOMICAL SOC PACIFIC , 2015, Vol. 497, p. 219-220Conference paper, Published paper (Refereed)
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Abstract [en]

We present new Herschel(1) HIFI (de Graauw et al. 2010) and PACS (Poglitsch et al. 2010) sub-millimeter and far-infrared line observations of several molecular species towards the S-type AGB star W Aql. We use these observations, which probe a wide range of gas temperatures, to constrain the circumstellar properties of W Aql, including mass-loss rate and molecular abundances.

Place, publisher, year, edition, pages
ASTRONOMICAL SOC PACIFIC , 2015. Vol. 497, p. 219-220
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:uu:diva-294836ISI: 000371098100042ISBN: 9781583818794 (print)OAI: oai:DiVA.org:uu-294836DiVA: diva2:953806
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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