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    15 years of very long baseline interferometry observations of two compact radio sources in Messier 82

    Access Status
    Open access via publisher
    Authors
    Beswick, R.
    Riley, J.
    Marti-Vidal, I.
    Pedlar, A.
    Muxlow, T.
    McDonald, A.
    Wills, K.
    Fenech, D.
    Argo, Megan
    Date
    2006
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Beswick, R. J. and Riley, J. D. and Marti-Vidal, I. and Pedlar, A. and Muxlow, T.W.B. and McDonald, A.R. and Wills, K.A. and Fenech, D. and Argo, M.K. 2006. 15 years of very long baseline interferometry observations of two compact radio sources in Messier 82. Monthly Notices of the Royal Astronomical Society. 369 (3): pp. 1221-1228.
    Source Title
    Monthly Notices of the Royal Astronomical Society
    DOI
    10.1111/j.1365-2966.2006.10363.x
    ISSN
    0035-8711
    Faculty
    Faculty of Science and Engineering
    Curtin Institute of Radio Astronomy
    URI
    http://hdl.handle.net/20.500.11937/12346
    Collection
    • Curtin Research Publications
    Abstract

    We present the results of a second epoch of 18-cm global very long baseline interferometry (VLBI) observations, taken on 2001 February 23, of the central kiloparsec of the nearby starburst galaxy Messier 82. These observations further investigate the structural and flux evolution of the most compact radio sources in the central region of M82. The two most compact radio objects in M82 have been investigated (41.95+575 and 43.31+592). Using this recent epoch of data in comparison with our previous global VLBI observations and two earlier epochs of European VLBI network observations, we measure expansion velocities in the range of 1500-2000 km s-1 for 41.95+575 and 9000-11 000 km s-1 for 43.31+592 using various independent methods. In each case, the measured remnant expansion velocities are significantly larger than the canonical expansion velocity (500 km s-1) of supernova remnants (SNRs) within M82 predicted from theoretical models. In this paper, we discuss the implications of these measured expansion velocities with respect to the high-density environment that the SNRs are expected to reside in within the centre of the M82 starburst.

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