Post-AGB stars in the LMC and SMC

H. Van Winckel, Els van Aarle, P. R. Wood, Devika Kamath, Tom Lloyd Evans, Kenneth De Smedt, Nadya Gorlova, Clio Gielen

    Research output: Chapter in Book/Report/Conference proceedingConference proceeding contribution

    Abstract

    Galactic post-AGB stars show a large diversity in chemical compositions as well as in the kinematical and geometrical properties of their circumstellar material. The theoretical interpretation is hampered by the lack of good distances to almost all Galactic objects. We therefore initiated a large project to study systematically post-AGB stars in the Large and Small Magellanic Cloud (LMC, SMC respectively). Here we report on our preliminary results.
    Original languageEnglish
    Title of host publicationPlanetary nebulae : an eye to the future
    Subtitle of host publicationproceedings of the 283rd Symposium of the International Astronomical Union held in Perto de la Cruz, Tenerife, Spain, July 25-29, 2011
    EditorsArturo Manchado, Letizia Stanghellini, Detlef Schönberner
    Place of PublicationCambridge
    PublisherCambridge University Press
    Pages235-238
    Number of pages4
    ISBN (Print)9781107019836
    DOIs
    Publication statusPublished - 2012
    Event283rd Symposium of the International Astronomical Union - Perto de la Cruz, Spain
    Duration: 25 Jul 201129 Jul 2011

    Publication series

    NameIAU symposium proceedings series
    PublisherCambridge University Press
    Number283
    ISSN (Print)1743-9213

    Conference

    Conference283rd Symposium of the International Astronomical Union
    Country/TerritorySpain
    CityPerto de la Cruz
    Period25/07/1129/07/11

    Keywords

    • Stars: AGB and post-AGB
    • stars: evolution
    • Magellanic Clouds
    • circumstellar matter

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