scholarly journals Relativistic electron production during driven magnetic reconnection

2006 ◽  
Vol 33 (13) ◽  
Author(s):  
P. L. Pritchett
2018 ◽  
Vol 98 (4) ◽  
Author(s):  
A. E. Raymond ◽  
C. F. Dong ◽  
A. McKelvey ◽  
C. Zulick ◽  
N. Alexander ◽  
...  

1973 ◽  
Author(s):  
D. A. Spong ◽  
J. F. Clarke ◽  
J. A. Rome

2019 ◽  
Vol 15 (S354) ◽  
pp. 189-194
Author(s):  
J. B. Climent ◽  
J. C. Guirado ◽  
R. Azulay ◽  
J. M. Marcaide

AbstractWe report the results of three VLBI observations of the pre-main-sequence star AB Doradus A at 8.4 GHz. With almost three years between consecutive observations, we found a complex structure at the expected position of this star for all epochs. Maps at epochs 2007 and 2010 show a double core-halo morphology while the 2013 map reveals three emission peaks with separations between 5 and 18 stellar radii. Furthermore, all maps show a clear variation of the source structure within the observing time. We consider a number of hypothesis in order to explain such observations, mainly: magnetic reconnection in loops on the polar cap, a more general loop scenario and a close companion to AB Dor A.


Sign in / Sign up

Export Citation Format

Share Document