Study of underground muons during the January 1991 radio flare of Cygnus X-3

1993 ◽  
Vol 47 (10) ◽  
pp. 4203-4205 ◽  
Author(s):  
R. Becker-Szendy ◽  
C. B. Bratton ◽  
D. Casper ◽  
S. T. Dye ◽  
W. Gajewski ◽  
...  
1991 ◽  
Vol 269 (1-2) ◽  
pp. 220-226 ◽  
Author(s):  
M.A. Thomson ◽  
J.H. Cobb ◽  
W.W.M. Allison ◽  
G.J. Alner ◽  
I. Ambats ◽  
...  

2007 ◽  
Vol 477 (1) ◽  
pp. 267-272 ◽  
Author(s):  
J. Forbrich ◽  
K. M. Menten ◽  
M. J. Reid
Keyword(s):  

1980 ◽  
Vol 88 ◽  
pp. 403-403
Author(s):  
Paul A. Feldman

For several years, a systematic program to observe RS CVn and similar binaries has been undertaken with the 46-m telescope of the Algonquin Radio Observatory. A number of large radio outbursts at 2.8 cm wavelength has been found from HR 1099, AR Lac, SZ Psc, UX Ari, and HR 5110. In several cases, simultaneous, or nearly simultaneous, observations of these stars were made by cooperating observers at (other) radio, optical, UV, and X-ray wavelengths. It is now clearly established that the mechanism responsible for the cm-wavelength radio emission is nonthermal gyrosynchrotron radiation in a volume whose characteristic dimension is comparable with the binary star separation. More generally, a semi-quantitative model for the radio flare activity of these stars seems to be possible using greatly scaled-up analogues of solar magnetic activity.


2006 ◽  
Vol 368 (2) ◽  
pp. 844-850 ◽  
Author(s):  
M. A. Worsley ◽  
A. C. Fabian ◽  
G. G. Pooley ◽  
C. J. Chandler
Keyword(s):  
X Ray ◽  

1973 ◽  
Vol 246 (155) ◽  
pp. 111-112 ◽  
Author(s):  
A. WOODSWORTH ◽  
V. A. HUGHES
Keyword(s):  

1990 ◽  
Vol 95 (A3) ◽  
pp. 2419 ◽  
Author(s):  
L. Bergamasco ◽  
A. Provenzale ◽  
G. Cini Castagnoli ◽  
M. Serio ◽  
V. A. Kudrjavtsev ◽  
...  

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