袁峰 教授 1997年中国科学技术大学博士 Email: fyuan@fudan.edu.cn 主要经历: 1994山东大学理论化学研究所硕士 1997中国科学技术大学天体物理中心博士 1998-2000南京大学天文系博士后 2000-2002德国马普射电天文研究所博士后 2002-2003美国哈佛大学哈佛-史密松天体物理中心博士后 2003-2005美国普渡大学物理系博士后 2005-2023中国科学院上海天文台研究员 2024至今beat365手机官方网站物理系教授 教学与研究领域: 活动星系核 星系形成与演化 计算天体物理 Feng Yuan Professor Ph.D(1997), University of Science and Technology of China Research Interests: Selected Publications: Yang, H., Yuan, F., Li, H., Mizuno, Y., Guo, F., Lu, R., Ho, L.C., Lin, Xi, Zdziarski, A.A., Wang, J. Modeling the inner part of M87 jet: confronting jet morphology with theory, 2024, Science Advances, 10, eadn3544 Lin, X., Yuan, F., Revisiting flares in Sagittarius A* based on general relativistic magnetohydrodynamic numerical simulations of black hole accretion, 2024, MNRAS, 531, 3136 Čemeljić, M., Yang, H., Yuan, F., Shang, H. Formation of Episodic Jets and Associated Flares from Black Hole Accretion Systems, 2022, ApJ, 933, 55 Shi, F., Li, Z., Yuan, F., Zhu, B. An energetic hot wind from the low-luminosity active galactic nucleus M81*, 2021, Nat. Ast. 5, 928 Yuan, F., Yoon, D., Li, Y., Gan, Z., Ho, L. & Guo, F. Active Galactic Nuclei Feedback in an Elliptical Galaxy with the Most Updated AGN Physics (I): Low-angular Momentum Case, 2018, ApJ, 857, 121 Yuan, F., Gan, Z.M., Narayan, R., Sadowski, A.,Bu, D., & Bai, X.-N. Numerical Simulation of Hot Accretion Flows (III): Revisiting wind properties using trajectory approach, 2015, ApJ, 804, 101 Yuan, F., Narayan, R. Hot Accretion Flows Around Black holes, 2014, ARA&A, 52,529 Yuan, F., Bu, D., & Wu, M. Numerical Simulation of Hot Accretion Flows (II): Nature, Origin, and Properties of Outflow and Their Possible Observational Applications, 2012, ApJ, 761,130 Yuan, F., Lin, J., Wu, K., & Ho, L. A Magnetohydrodynamical Model for the Formation of Episodic Jets, 2009, MNRAS, 395, 2183. Yuan, F., Quataert, E., & Narayan, R. Nonthermal Electrons in Radiatively Inefficient Accretion Flow Models of Sagittarius A*, 2003, ApJ, 598, 301
1991山东大学物理系学士
黑洞吸积与外流理论
Black hole accretion and outflow; active galactic nuclei; galaxy formation and evolution; computational astrophysics