Dwarf nova-type cataclysmic variable stars are significant radio emitters
We present 8–12 GHz radio light curves of five dwarf nova (DN) type cataclysmic variable stars (CVs) in outburst (RX And, U Gem, and Z Cam), or superoutburst (SU UMa and YZ Cnc), increasing the number of radio-detected DN by a factor of 2. The observed radio emission was variable on time-scales of m...
| Main Authors: | Coppejans, D., Kording, E., Miller-Jones, James, Rupen, M., Sivakoff, G., Knigge, C., Groot, P., Woudt, P., Waagen, E., Templeton, M. |
|---|---|
| Format: | Journal Article |
| Published: |
Oxford University Press
2016
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| Online Access: | http://purl.org/au-research/grants/arc/FT140101082 http://hdl.handle.net/20.500.11937/50765 |
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