【特邀报告】An Off-Axis Corona Model for X-Ray Binaries
中国科学院云南天文台特邀学术报告
YNAO Colloquium 2026
第9期
报告题目:An Off-Axis Corona Model for X-Ray Binaries
报告人单位:中国科学技术大学
报告语言:中文
报告时间:2026年5月28日(星期四)10:30-12:00
报告地点:科研7号楼2楼阶梯教室
主持人:陈雪飞
Abstract:
~~~~~~~~~~~~~
Characteristic reflection features are frequently observed in the X-ray spectra of accreting black holes. This reflected emission primarily originates from the innermost region of the accretion disk and is shaped by relativistic effects in the strong gravitational field around the black hole. In this talk, I will present our investigation of the reflection features produced when the accretion disk is illuminated by a corona offset from the black hole’s spin axis, and discuss its implications for the spectral measurements of X-ray binaries.
~~~~~~~~~~~~~
Speaker:
Dr. Ye-Fei Yuan is currently a Chair Professor at the University of Science and Technology of China (USTC). He received his PhD from the USTC Center for Astrophysics in 1999 and subsequently joined the faculty of the Department of Astronomy at USTC. His research focuses on the dynamics and emissions near black hole event horizons.
主办:中国科学院云南天文台学术委员会
联系人:柳正伟
附件下载: