On the natural line width of absorption lines in strong magnetic stellar fields

1994 ◽  
Vol 214 (1-2) ◽  
pp. 103-114
Author(s):  
Javier Bonatti

Author(s):  
L.F. Vitushkin ◽  
S.V. Lazaryuk ◽  
S.A. Pul'kin ◽  
L. Robertsson ◽  
M.Z. Smirnov ◽  
...  


1959 ◽  
Vol 129 ◽  
pp. 456 ◽  
Author(s):  
G. Breit ◽  
M. H., Jr. Hull


2010 ◽  
Vol 206 (1) ◽  
pp. 168-170 ◽  
Author(s):  
H. Harcken ◽  
R. Ketzler ◽  
M. Albrecht ◽  
M. Burghoff ◽  
S. Hartwig ◽  
...  


1970 ◽  
Vol 32 (5) ◽  
pp. 399-403 ◽  
Author(s):  
G. Backenstoss ◽  
A. Bamberger ◽  
J. Egger ◽  
W.D. Hamilton ◽  
H. Koch ◽  
...  






1970 ◽  
Vol 25 (12) ◽  
pp. 1779-1780 ◽  
Author(s):  
B. Wolbeck ◽  
K . Zioutas

Abstract The Mößbauer effect of the 129 keV transition in 195Pt has been observed. By use of a Ge(Li) detector any contribution from the strong 99 keV Mößbauer line could be eliminated. The width of the resonance absorption line corresponds to the natural line width. We derived from the magnitude of the observed Mößbauer effect the branching ratio in the decay of the 129 keV level as I (129)/I (31) = ( 5.7 ± 1.6)% .



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