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Unraveling Disks In Agb Stars
Univ Vienna, Inst Astron, A-1010 Vienna, Austria..
Univ Vienna, Inst Astron, A-1010 Vienna, Austria..
Jodrell Bank Ctr Astrophys, Macclesfield, Cheshire, England..
Sydney Inst Astron, Sydney, NSW, Australia..
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2015 (English)In: Physics Of Evolved Stars: A Conference Dedicated To The Memory Of Olivier Chesneau / [ed] Lagadec, E; Millour, F, EDP Sciences, 2015, 217-222 p.Conference paper, Published paper (Refereed)
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Abstract [en]

It is commonly accepted that asymmetries found in the post-AGB stars and planetary nebulae should originate as early as during the AGB phase. We present results from our high-angular resolution observing programs, with an aperture masking technique on the VLT, of a sample of evolved stars that were known to present asymmetries at larger spatial scales (e.g. jets, torii and/or bipolar nebulae). Disk-like structures have been found in the vicinity of at least two of these stars.

Place, publisher, year, edition, pages
EDP Sciences, 2015. 217-222 p.
Series
EAS Publications Series, ISSN 1633-4760 ; 71-72
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:uu:diva-284911DOI: 10.1051/eas/1571049ISI: 000370302700048ISBN: 978-2-7598-1907-2 (print)OAI: oai:DiVA.org:uu-284911DiVA: diva2:920968
Conference
Physics of Evolved Stars: A Conference Dedicated to the Memory of Olivier Chesneau, JUN 08, 2015, Nice, FRANCE
Available from: 2016-04-19 Created: 2016-04-19 Last updated: 2016-04-19Bibliographically approved

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Ramstedt, Sofia

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