The reproducible radio outbursts of SS Cygni

The reproducible radio outbursts of SS Cygni

We present the results of our intensive radio observing campaign of the dwarf nova SS Cyg during its 2010 April outburst. We argue that the observed radio emission was produced by synchrotron emission from a transient radio jet. Comparing the radio light curves from previous and subsequent outbursts...

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Bibliographic Details
Main Authors: Russell, T., Miller-Jones, James, Sivakoff, G., Altamirano, D., O'Brien, T., Page, K., Templeton, M., Körding, E., Knigge, C., Rupen, M., Fender, R., Heinz, S., Maitra, D., Markoff, S., Migliari, S., Remillard, R., Russell, D., Sarazin, C., Waagen, E.
Format: Journal Article
Published: Oxford University Press 2016
Online Access:http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/22970

Internet

http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/22970

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