Planetary nebulae in the VISTA Magellanic Cloud (VMC) Survey

Brent Miszalski*, Ralph Napiwotzki, Maria Rosa L. Cioni, Martin A.T. Groenewegen, Jose M. Oliveira, Andrzej Udalski, Jia Cai Nie

*Corresponding author for this work

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

    Abstract

    The multi-epoch YJK s sub-arcsecond photometry of the VMC survey provides a long anticipated deep near-infrared (NIR) window into further understanding the stellar populations of the Magellanic Clouds. The first year of observations consisted of six tiles covering ∼9% of the Large Magellanic Cloud (LMC) survey region and contains 102 objects previously classified as planetary nebulae (PNe). A large proportion of the sample were found to be contaminated by non-PNe. These initial results underline the importance of establishing a clean catalogue of LMC PNe before they are applied in areas such as the planetary nebula luminosity function (PNLF) and searches for binary central stars. As the VMC survey progresses it will play a fundamental role in cleaning extant PN catalogues and a complementary role in the discovery of new PNe.

    Original languageEnglish
    Title of host publicationPlanetary Nebulae
    Subtitle of host publicationAn Eye to the Future
    PublisherCambridge University Press
    Pages444-445
    Number of pages2
    EditionS283
    ISBN (Print)9781107019836
    DOIs
    Publication statusPublished - Jul 2011

    Publication series

    NameProceedings of the International Astronomical Union
    NumberS283
    Volume7
    ISSN (Print)1743-9213
    ISSN (Electronic)1743-9221

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