Measurement and analysis of argon continuum radiation from a 12-CM diameter gas puff Z pinch at 6MA

2006 ◽  
Author(s):  
F.C. Young ◽  
J.P Apruzese ◽  
R.J. Commisso ◽  
D. Mosher ◽  
D.P. Murphy ◽  
...  
Keyword(s):  
Continuum Radiation ◽  
Measurement And Analysis ◽  
Z Pinch

Measurement and Analysis of Continuum Radiation From a Large-Diameter Long Implosion Time Argon Gas Puff$Z$-Pinch at 6 MA

2006 ◽  
Vol 34 (5) ◽  
pp. 2312-2324 ◽  
Author(s):  
F.C. Young ◽  
R.J. Commisso ◽  
D.P. Murphy ◽  
J.P. Apruzese ◽  
D. Mosher ◽  
...  
Keyword(s):  
Large Diameter ◽  
Argon Gas ◽  
Continuum Radiation ◽  
Measurement And Analysis ◽  
Z Pinch

Theory of High-Energy-Photon K-Shell Recombination Continuum Radiation From $Z$-Pinch Plasmas

2010 ◽  
Vol 38 (4) ◽  
pp. 618-625 ◽  
Author(s):  
Alexander L Velikovich ◽  
John P Apruzese ◽  
Jack Davis ◽  
J Ward Thornhill
Keyword(s):  
High Energy ◽  
High Energy Photon ◽  
Energy Photon ◽  
Continuum Radiation ◽  
Z Pinch

Iron K-Line Emission from X-Ray Binaries

1988 ◽  
Vol 102 ◽  
pp. 47-50
Author(s):  
K. Masai ◽  
S. Hayakawa ◽  
F. Nagase
Keyword(s):  
Accretion Disk ◽  
Radiative Recombination ◽  
Characteristic Temperature ◽  
Line Emission ◽  
Ionization Front ◽  
Continuum Radiation ◽  
X Ray ◽  
Low Mass ◽  
X Ray Binaries

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.

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