Band structure enhancement and optimization of radiative recombination in GaAs1−x Px:N (and In1−x Gax P:N)

1974 ◽  
Vol 45 (10) ◽  
pp. 4543-4553 ◽  
Author(s):  
J. C. Campbell ◽  
N. Holonyak ◽  
M. G. Craford ◽  
D. L. Keune
1977 ◽  
Vol 21 (5) ◽  
pp. 437-439 ◽  
Author(s):  
D. Auvergne ◽  
P. Merle ◽  
H. Mathieu

1979 ◽  
Vol 20 (12) ◽  
pp. 5292-5296 ◽  
Author(s):  
J. Camassel ◽  
J. Pascual ◽  
H. Mathieu

1964 ◽  
Vol 13 (2) ◽  
pp. 103-105 ◽  
Author(s):  
F.A. Junga ◽  
K.F. Cuff ◽  
J.S. Blakemore ◽  
E.R. Washwell

1988 ◽  
Vol 102 ◽  
pp. 47-50
Author(s):  
K. Masai ◽  
S. Hayakawa ◽  
F. Nagase

AbstractEmission mechanisms of the iron Kα-lines in X-ray binaries are discussed in relation with the characteristic temperature Txof continuum radiation thereof. The 6.7 keV line is ascribed to radiative recombination followed by cascades in a corona of ∼ 100 eV formed above the accretion disk. This mechanism is attained for Tx≲ 10 keV as observed for low mass X-ray binaries. The 6.4 keV line observed for binary X-ray pulsars with Tx> 10 keV is likely due to fluorescence outside the He II ionization front.


Physica ◽  
1954 ◽  
Vol 3 (7-12) ◽  
pp. 967-970
Author(s):  
D JENKINS

1976 ◽  
Vol 37 (2) ◽  
pp. 149-158 ◽  
Author(s):  
A.K. Bhattacharjee ◽  
B. Caroli ◽  
D. Saint-James
Keyword(s):  

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