Inverse-synchrotron-radiation electron acceleration.

1990 ◽  
Vol 2 (3) ◽  
pp. 185-188
Author(s):  
Hiroaki Watanabe ◽  
Atushi Manabe ◽  
Shigeo Kawata
2010 ◽  
Vol 6 (S272) ◽  
pp. 638-639 ◽  
Author(s):  
Delia Volpi ◽  
Ronny Blomme ◽  
Michael De Becker ◽  
Gregor Rauw

AbstractSome OB stars show variable non-thermal radio emission. The non-thermal emission is due to synchrotron radiation that is emitted by electrons accelerated to high energies. The electron acceleration occurs at strong shocks created by the collision of radiatively-driven stellar winds in binary systems. Here we present results of our modelling of two colliding wind systems: Cyg OB2 No. 8A and Cyg OB2 No. 9.


New Astronomy ◽  
1998 ◽  
Vol 3 (3) ◽  
pp. 157-173 ◽  
Author(s):  
Charles D. Dermer ◽  
James Chiang

1990 ◽  
Vol 29 (Part 2, No. 1) ◽  
pp. L179-L181 ◽  
Author(s):  
Shigeo Kawata ◽  
Hiroaki Watanabe ◽  
Atsushi Manabe ◽  
Hiroto Kuroda

Author(s):  
B. Jouffrey ◽  
D. Dorignac ◽  
A. Bourret

Since the early works on GP zones and the model independently proposed by Preston and Guinier on the first steps of precipitation in supersaturated solid solution of aluminium containing a few percent of copper, many works have been performed to understand the structure of different stages in the sequence of precipitation.The scheme which is generally admitted can be drawn from a work by Phillips.In their original model Guinier and Preston analysed a GP zone as composed of a single (100) copperrich plane surrounded by aluminum atomic planes with a slightly shorter distance from the original plane than in the solid solution.From X-ray measurements it has also been shown that GP1 zones were not only copper monolayer zones. They could be up to a few atomic planes thick. Different models were proposed by Guinier, Gerold, Toman. Using synchrotron radiation, proposals have been recently made.


2005 ◽  
Vol 25 (1_suppl) ◽  
pp. S558-S558
Author(s):  
Masahiro Tamaki ◽  
Takashi Mizobe ◽  
Keiji Kidoguchi ◽  
Junnji Koyama ◽  
Takeshi Kondoh ◽  
...  

1973 ◽  
Vol 34 (C8) ◽  
pp. C8-63-C8-63
Author(s):  
J. BARRINGTON LEIGH ◽  
G. ROSENBAUM

1987 ◽  
Vol 48 (C1) ◽  
pp. C1-175-C1-181
Author(s):  
S. AHMAD ◽  
M. OHTOMO ◽  
R. W. WHITWORTH

1988 ◽  
Vol 49 (C8) ◽  
pp. C8-1891-C8-1892
Author(s):  
J. Baruchel ◽  
M. Schlenker ◽  
J. Sandonis

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