Improved Reflection Models of Black Hole Accretion Disks: Treating the Angular Distribution of X- Rays

Improved Reflection Models of Black Hole Accretion Disks: Treating the Angular Distribution of X- RaysDOI: info:10.1088/0004-637X/782/2/76v. 78276
GarcĂ­a, J., Dauser, T., Lohfink, A., Kallman, T. R., Steiner, J. F., McClintock, J. E., Brenneman, L., Wilms, J., Eikmann, W., Reynolds, C. S., and Tombesi, F. 2014. "Improved Reflection Models of Black Hole Accretion Disks: Treating the Angular Distribution of X- Rays." The Astrophysical Journal, 782 76. https://doi.org/10.1088/0004-637X/782/2/76.
ID: 119060
Type: article
Keywords: SAO