Reverse and Forward Shock X-Ray Emission in an Evolutionary Model of Supernova Remnants Undergoing Efficient Diffusive Shock Acceleration

Reverse and Forward Shock X-Ray Emission in an Evolutionary Model of Supernova Remnants Undergoing Efficient Diffusive Shock AccelerationDOI: info:10.1088/0004-637X/791/2/97v. 79197
Lee, Shiu-Hang, Patnaude, Daniel J., Ellison, Donald C., Nagataki, Shigehiro, and Slane, Patrick O. 2014. "Reverse and Forward Shock X-Ray Emission in an Evolutionary Model of Supernova Remnants Undergoing Efficient Diffusive Shock Acceleration." The Astrophysical Journal, 791 97. https://doi.org/10.1088/0004-637X/791/2/97.
ID: 128140
Type: article
Keywords: SAO