853 citations · 7.8k across the 120 of their papers we have counts for
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Shock-powered radio emission from V5589 Sagittarii (Nova Sgr 2012 1)
Jennifer H. S. Weston, J. L. Sokoloski, Laura Chomiuk +7
Since the Fermi discovery of -rays from novae, one of the biggest questions in the field has been how novae generate such high-energy emission. Shocks must be a fundamental ingr…
Magnetospherically driven optical and radio aurorae at the end of the stellar main sequence
G. Hallinan, S. P. Littlefair, G. Cotter +12
Aurorae are detected from all the magnetized planets in our Solar System, including Earth. They are powered by magnetospheric current systems that lead to the precipitation of ener…
Novalike Cataclysmic Variables are Significant Radio Emitters
Deanne L. Coppejans, Elmar G. Koerding, James C. A. Miller-Jones +4
Radio emission from non-magnetic cataclysmic variables (CVs, accreting white dwarfs) could allow detailed studies of outflows and possibly accretion flows in these nearby, numerous…
Non-Thermal Radio Emission from Colliding Flows in Classical Nova V1723 Aql
Jennifer H. S. Weston, J. L. Sokoloski, Brian D. Metzger +9
The importance of shocks in nova explosions has been highlighted by Fermi's discovery of γ-ray producing novae. Over three years of multi-band VLA radio observations of the 2010 no…
Imaging the Expanding Shell of SN 2011dh
A. de Witt, M. F. Bietenholz, A. Kamble +5
We report on third epoch VLBI observations of the radio-bright supernova SN 2011dh located in the nearby (7.8 Mpc) galaxy M51. The observations took place at d after the ex…
Thermal radio emission from novae & symbiotics with the Square Kilometre Array
Tim O'Brien, Michael Rupen, Laura Chomiuk +4
The thermal radio emission of novae during outburst enables us to derive fundamental quantities such as the ejected mass, kinetic energy, and density profile of the ejecta. Recent…