Figure 9 from A SPATIALLY RESOLVED STUDY OF THE SYNCHROTRON EMISSION AND TITANIUM IN TYCHO’S SUPERNOVA REMNANT USING NuSTAR

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A SPATIALLY RESOLVED STUDY OF THE SYNCHROTRON EMISSION AND TITANIUM IN TYCHO’S SUPERNOVA REMNANT USING NuSTAR

Authors: Laura A. Lopez, Brian W. Grefenstette, Stephen P. Reynolds, Hongjun An, Steven E. Boggs, Finn E. Christensen, William W. Craig, Kristoffer A. Eriksen, Chris L. Fryer, Charles J. Hailey, Fiona A. Harrison, Kristin K. Madsen, Daniel K. Stern, William W. Zhang, and Andreas Zoglauer

2015 The Astrophysical Journal 814 132.

Provider: AAS Journals

Caption: Figure 9.

Example spectra and fits using an absorbed srcut model for six regions. Although the spectra were fit over the range 10–50 keV where the non-thermal emission dominates, the spectra above span 3–50 keV to demonstrate the adequacy of the srcut model at predicting the non-thermal continuum across this energy range.

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