This decommissioned ERA site remains active temporarily to support our final migration steps to https://ualberta.scholaris.ca, ERA's new home. All new collections and items, including Spring 2025 theses, are at that site. For assistance, please contact erahelp@ualberta.ca.
Search
Skip to Search Results- 2Fender, Rob P.
- 2Russell, Thomas D.
- 2Sivakoff, Gregory Robert
- 2Waagen, Elizabeth O.
- 1Altamirano, Diego
- 1Carey, S. H.
- 2Radio Continuum: Stars
- 2X-Rays: Stars
- 1Cataclysmic Variables
- 1Novae
- 1Stars: Dwarf Novae
- 1Stars: Individual: (Ss Cygni)
-
2017-01-01
Mooley, Kunal. P., Miller-Jones, James. C. A., Fender, Rob P., Sivakoff, Gregory Robert, Rumsey, C., Perrott, Y., Titterington, David, Grainge, K. J. B., Russell, Thomas D., Carey, S. H., Hickish, Jack, Razavi-Ghods, Nima, Scaife, A., Scott, P., Waagen, Elizabeth O.
The connection between accretion and jet production in accreting white dwarf binary systems, especially dwarf novae, is not well understood. Radio wavelengths provide key insights into the mechanisms responsible for accelerating electrons, including jets and outflows. Here, we present densely...
-
2016-01-01
Russell, Thomas D., Miller-Jones, James C. A., Sivakoff, Gregory Robert, Altamirano, Diego, O'Brien, Tim J., Page, Kim L., Templeton, Matthew R., Körding, E. G., Knigge, C., Fender, Rob P., Heinz, S., Maitra, D., Markoff, Sera, Rupen, Michael P., Migliari, Simone, Remillard, Ronald Alan, Russell, D. M., Sarazin, Craig L., Waagen, Elizabeth O.
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...