Muon Lifetime Measurement with the FAST Experiment: First Results

2008 ◽  
Author(s):  
M. Chiara Casella ◽  
Osamu Yasuda ◽  
Naba Mondal ◽  
Chihiro Ohmori
2005 ◽  
Vol 149 ◽  
pp. 341-343 ◽  
Author(s):  
D. Tomono ◽  
S.N. Nakamura ◽  
Y. Matsuda ◽  
M. Iwasaki ◽  
G. Mason ◽  
...  

2008 ◽  
Author(s):  
L. Villaseñor ◽  
Heriberto Castilla-Valdez ◽  
Omar Miranda ◽  
Eli Santos

2000 ◽  
Author(s):  
Serkant Ali Çetin

1998 ◽  
Author(s):  
Luis Villaseñor

2017 ◽  
Vol 866 ◽  
pp. 012011
Author(s):  
Luis Rodolfo Pérez Sánchez ◽  
Federico Izraelevitch

1976 ◽  
Vol 32 ◽  
pp. 577-588
Author(s):  
C. Mégessier ◽  
V. Khokhlova ◽  
T. Ryabchikova

My talk will be on the oblique rotator model which was first proposed by Stibbs (1950), and since received success and further developments. I shall present two different attempts at describing a star according to this model and the first results obtained in the framework of a Russian-French collaboration in order to test the precision of the two methods. The aim is to give the best possible representation of the element distributions on the Ap stellar surfaces. The first method is the mathematical formulation proposed by Deutsch (1958-1970) and applied by Deutsch (1958) to HD 125248, by Pyper (1969) to α2CVn and by Mégessier (1975) to 108 Aqr. The other one was proposed by Khokhlova (1974) and used by her group.


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