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NT Ingolia, AW Murray - Science, 2002 - science.org
Science, 2002•science.org
Iron lines in stellar mass black holes.(Red) Ratio of the spectrum of XTE J1650-500
(observed with XMM-Newton) to a simple disk blackbody and power law.(Blue) Same ratio
for Cygnus X-1 (from Chandra). Plotting the spectrum in this manner reveals the shape of the
iron line, which can be seen as a broad bump between 4 and 7 keV.[Data from (7)]
(observed with XMM-Newton) to a simple disk blackbody and power law.(Blue) Same ratio
for Cygnus X-1 (from Chandra). Plotting the spectrum in this manner reveals the shape of the
iron line, which can be seen as a broad bump between 4 and 7 keV.[Data from (7)]
Iron lines in stellar mass black holes.(Red) Ratio of the spectrum of XTE J1650-500 (observed with XMM-Newton) to a simple disk blackbody and power law.(Blue) Same ratio for Cygnus X-1 (from Chandra). Plotting the spectrum in this manner reveals the shape of the iron line, which can be seen as a broad bump between 4 and 7 keV.[Data from (7)]
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