Observing third dredge up in NGC 1846

T. Lebzelter*, K. H. Hinkle, M. T. Lederer, S. Cristallo, O. Straniero, W. Nowotny, P. Wood

*Corresponding author for this work

    Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

    Abstract

    In this contribution we present the first measurements of the C/O ratio for a sample of AGB stars in the LMC globular cluster NGC 1846. From a variability study we set strong constraints on the mass of the cluster stars, which is an important quantity for comparison with evolutionary models. Variations of the surface abundance both with luminosity and pulsation properties were found and the various relevant factors are discussed. We find a good agreement with our synthetic models if we assume [O/Fe]=±0.2dex. The F abundance seems to increase with the C/O ratio. As variability plays a key role on the AGB we give some preliminary results from our study of abundance determination in the dynamical case at the end of this paper.

    Original languageEnglish
    Title of host publicationNinth Torino Workshop on Evolution and Nucleosynthesis in AGB Stars and the Second Perugia Workshop on Nuclear Astrophysics
    Pages56-62
    Number of pages7
    DOIs
    Publication statusPublished - 2008
    Event9th Torino Workshop on Evolution and Nucleosynthesis in AGB Stars and the 2nd Perugia Workshop on Nuclear Astrophysics - Perugia, Italy
    Duration: 21 Oct 200727 Oct 2007

    Publication series

    NameAIP Conference Proceedings
    Volume1001
    ISSN (Print)0094-243X
    ISSN (Electronic)1551-7616

    Conference

    Conference9th Torino Workshop on Evolution and Nucleosynthesis in AGB Stars and the 2nd Perugia Workshop on Nuclear Astrophysics
    Country/TerritoryItaly
    CityPerugia
    Period21/10/0727/10/07

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