Search Results - Waagen, E.

An accurate geometric distance to the compact binary SS Cygni vindicates accretion disc theory by Miller-Jones, James, Sivakoff, G., Knigge, C., Koerding, E., Templeton, M., Waagen, E.

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Dwarf nova-type cataclysmic variable stars are significant radio emitters by Coppejans, D., Kording, E., Miller-Jones, James, Rupen, M., Sivakoff, G., Knigge, C., Groot, P., Woudt, P., Waagen, E., Templeton, M.

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Rapid radio flaring during an anomalous outburst of SS Cyg by Mooley, K., Miller-Jones, James, Fender, R., Sivakoff, G., Rumsey, C., Perrott, Y., Titterington, D., Grainge, K., Russell, T., Carey, S., Hickish, J., Razavi-Ghods, N., Scaife, A., Scott, P., Waagen, E.

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The reproducible radio outbursts of SS Cygni by 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.

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