Rikkyo University (Tokyo), October 21-22 2015
✔Accretion and Winds
✔Photoionized plasma from theory and lab
✔Modeling of spectra
Tadayuki Takahashi (ISAS/JAXA), Yasunobu Uchiyama (Rikkyo University)
Dmitry Khangulyan (Rikkyo University), Anton Dorodnitsyn (GSFC/NASA)
AGN is a multi-scale phenomenon with different parts coupled by intense radiation and winds. Due to limitations of currently operating instruments, many details of this complex interplay remain a mystery. Drastic changes in this field are anticipated in the near future: observations with the calorimeter onboard of ASTRO-H will take studies of AGN to the next level. This presents an unprecedented opportunity to advance theoretical understanding of how these complex machines work. The goal of the workshop is to discuss the current state as well as the prospects of AGN modeling in the upcoming era of ASTRO-H.
Ken EBISAWA, Matteo GUAINAZZI, Kouichi HAGINO, Shigenobu HIROSE, Kohei ICHIKAWA, Yoshiyuki INOUE, Tim KALLMAN, Norita KAWANAKA, Kazuo MAKISHIMA, Hirofumi NODA, Mariko NOMURA, Hiro ODAKA, Ken OHSUGA, John SILVERMAN, Yoshihiro UEDA