The spectral energy distribution of powerful starburst galaxies - I. Modelling the radio continuum

The spectral energy distribution of powerful starburst galaxies - I. Modelling the radio continuum

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 c...

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Bibliographic Details
Main Authors: Galvin, T., Seymour, Nick, Marvil, J., Filipovic, M., Tothill, N., McDermid, R., Hurley-Walker, Natasha, Hancock, Paul, Callingham, J., Cook, R., Norris, R., Bell, M., Dwarakanath, K., For, B., Gaensler, B., Hindson, L., Johnston-Hollitt, Melanie, Kapinska, A., Lenc, E., McKinley, B., Morgan, John, Offringa, A., Procopio, P., Staveley-Smith, L., Wayth, Randall, Wu, C., Zheng, Q.
Format: Journal Article
Published: Oxford University Press 2018
Online Access:http://hdl.handle.net/20.500.11937/66555

Internet

http://hdl.handle.net/20.500.11937/66555

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