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    Galactic synchrotron emissivity measurements between 250° < l < 355° from the GLEAM survey with the MWA

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    250879 Erratum.pdf (740.8Kb)
    Access Status
    Open access
    Authors
    Su, H.
    Hurley-Walker, Natasha
    Jackson, Carole
    McClure-Griffiths, N.
    Tingay, Steven
    Hindson, L.
    Hancock, P.
    Wayth, Randall
    Gaensler, B.
    Staveley-Smith, L.
    Morgan, J.
    Johnston-Hollitt, M.
    Lenc, E.
    Bell, M.
    Callingham, J.
    Dwarkanath, K.
    For, B.
    Kapinska, A.
    McKinley, B.
    Offringa, A.
    Procopio, P.
    Wu, C.
    Zheng, Q.
    Date
    2017
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Su, H. and Hurley-Walker, N. and Jackson, C. and McClure-Griffiths, N. and Tingay, S. and Hindson, L. and Hancock, P. et al. 2017. Galactic synchrotron emissivity measurements between 250° < l < 355° from the GLEAM survey with the MWA. Monthly Notices of the Royal Astronomical Society. 465 (3): pp. 3163-3174.
    Source Title
    Monthly Notices of the Royal Astronomical Society
    DOI
    10.1093/mnras/stw2959
    ISSN
    0035-8711
    School
    Curtin Institute of Radio Astronomy (Physics)
    Remarks

    This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. © 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

    URI
    http://hdl.handle.net/20.500.11937/51676
    Collection
    • Curtin Research Publications
    Abstract

    Synchrotron emission pervades the Galactic plane at low radio frequencies, originating from cosmic ray electrons interacting with the Galactic magnetic field. Using a low-frequency radio telescope, the Murchison Widefield Array (MWA), we measure the free-free absorption of this Galactic synchrotron emission by intervening HII regions along the line of sight. These absorption measurements allow us to calculate the Galactic cosmic ray electron emissivity behind and in front of 47 detected HII regions in the region 250° < l < 355°, |b| < 2°.We find that all average emissivities between the HII regions and the Galactic edge along the line of sight (eb) are in the range of 0.39 ~ 1.45 K pc-1 with a mean of 0.77 K pc-1 and a variance of 0.14 K pc-1 at 88 MHz. Our best model, the two-circle model, divides the Galactic disc into three regions using two circles centring on the Galactic Centre. It shows a high emissivity region near the Galactic Centre, a low emissivity region near the Galactic edge, and a medium emissivity region between these two regions, contrary to the trend found by previous studies.

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