Global VLBI observations of M82

A R McDonald, T W B Muxlow, A Pedlar, M A Garrett, K A Wills, S T Garrington, P J Diamond, Una Hwang, Stephen S Holt (Editor)

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

    Abstract

    Images of the starburst galaxy M82 from a 20-station global VLBI experiment are presented with an angular resolution of up to 3 mas. These images resolve several of the sources into a number of components and with future VLBI experiments the expansion of these components may be tracked on a ~2 year timescale. Expansion of one of the brightest remnants in M82 has already been measured on a ~10 year timescale using the European VLBI Network (EVN) alone and an expansion rate of 10,000 km per second calculated. Furthermore, limits on the deceleration of this remnant have been deduced. Further VLBI experiments will be able to better constrain the deceleration of the remnants on a ~10 year timescale as they continue to interact with the interstellar medium in M82.
    Original languageEnglish
    Title of host publicationhost publication
    EditorsR T Schilizzi
    Place of PublicationManchester, UK
    Pages441-444
    Number of pages4
    Volume205
    Publication statusPublished - 2001
    EventGalaxies and their Constituents at the Highest Angular Resolutions -
    Duration: 1 Jan 1824 → …
    http://adsabs.harvard.edu/abs/2001IAUS..205..376M

    Conference

    ConferenceGalaxies and their Constituents at the Highest Angular Resolutions
    Period1/01/24 → …
    Internet address

    Keywords

    • Supernova remnants
    • Star formation
    • Interferometry

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