1988 ◽  
Vol 37 (18) ◽  
pp. 10862-10866 ◽  
Author(s):  
A. P. Marchetti ◽  
M. Burberry

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.


1982 ◽  
Vol 43 (2) ◽  
pp. 323-328 ◽  
Author(s):  
M.A. Khan ◽  
R. Riedinger
Keyword(s):  

1971 ◽  
Vol 32 (C1) ◽  
pp. C1-794-C1-795
Author(s):  
J. F. DILLON ◽  
Jr ◽  
E. M. GYORGY ◽  
J. P. REMEIKA

1971 ◽  
Vol 32 (C4) ◽  
pp. C4-236-C4-240 ◽  
Author(s):  
R. HAENSEL ◽  
G. KEITEL ◽  
N. KOSUCH ◽  
U. NIELSEN ◽  
P. SCHREIBER
Keyword(s):  

1976 ◽  
Vol 37 (C7) ◽  
pp. C7-203-C7-203
Author(s):  
P. KOIDL
Keyword(s):  

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