Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/6841
Title: The spectral energy distribution of powerful starburst galaxies – I. Modelling the radio continuum
Authors: Galvin, T.J.
Seymour, N.
Dwarakanath, K.S.
+23 Co-authors
Keywords: Galaxies Starburst
Radio continuum
Issue Date: Feb-2018
Publisher: Oxford University Press for The Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, 2018, Vol. 474, p779-799
Abstract: We have acquired radio-continuum data between 70 MHz and 48 GHz for a sample of 19 southern starburst galaxies at moderate redshifts (0.067 < z < 0.227) with the aim of separating synchrotron and free–free emission components. Using a Bayesian framework, we find the radio continuum is rarely characterized well by a single power law, instead often exhibiting low-frequency turnovers below 500 MHz, steepening at mid to high frequencies, and a flattening at high frequencies where free–free emission begins to dominate over the synchrotron emission. These higher order curvature components may be attributed to free–free absorption across multiple regions of star formation with varying optical depths. The decomposed synchrotron and free–free emission components in our sample of galaxies form strong correlations with the total-infrared bolometric luminosities. Finally, we find that without accounting for free–free absorption with turnovers between 90 and 500 MHz the radio continuum at low frequency (ν < 200 MHz) could be overestimated by upwards of a factor of 12 if a simple power-law extrapolation is used from higher frequencies. The mean synchrotron spectral index of our sample is constrained to be α = −1.06, which is steeper than the canonical value of −0.8 for normal galaxies. We suggest this may be caused by an intrinsically steeper cosmic ray distribution.
Description: Open Access
URI: http://hdl.handle.net/2289/6841
ISSN: 0035-8711
1365-2966 - (online)
Alternative Location: http://adsabs.harvard.edu/abs/2018MNRAS.474..779G
http://arxiv.org/abs/1710.01967
http://dx.doi.org/10.1093/mnras/stx2613
Copyright: 2018 The authors
Appears in Collections:Research Papers (A&A)

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