Molecular LineObservations of the Tornado Nebula and its Eye

J. Lazendic*, M. Burton, F. Yusef-Zadeh, M. Wardle, A. Green, J. Whiteoak

*Corresponding author for this work

    Research output: Contribution to journalArticlepeer-review

    3 Citations (Scopus)


    We present millimetre and NIR molecular-line observations of the Tornado Nebula and its Eye. The observations were motivated by the presence of OH(1720 MHz) maser emission towards the nebula, believed to be an indicator of interaction between a supernova remnant and a molecular cloud. We found that the distribution of molecular gas around the Tornado complements its radio morphology, implying that the nebula's appearance has been influenced by the structure of the surrounding molecular gas. Our NIR H2 observations revealed the presence of shocked molecular gas at the location where the nebula is expanding into the surrounding molecular cloud. It has been suggested that the Eye of the Tornado is related to the nebula on the basis of their apparent proximity. Our NIR and millimetre-line observations show that the two objects are not spatially related. Brγ line emission, in conjunction with IR data at longer wavelengths and high-resolution radio continuum observations, suggests that the Eye is a massive protostellar source deeply embedded within a dense molecular core.

    Original languageEnglish
    Pages (from-to)157-160
    Number of pages4
    JournalAstronomische Nachrichten
    Issue numberSUPPL.1
    Publication statusPublished - Sep 2003


    • Eye of Tornado
    • G357.63-0.06
    • G357.7-0.1
    • Molecular clouds
    • Shock waves
    • Star formation
    • Supernova remnants
    • Tornado Nebula


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