简　　历：

1999年-2004年中国科学技术大学本科（天文专业）；2004年-2009年中科院上海天文台博士（天体物理）；2009年至今在中科院上海天文台天体物理研究室工作，现为研究员，研究室副主任。另2009年-2011年在北京大学科维理天文与天体物理研究所开展博士后工作。

研究方向：

主要从事黑洞吸积的理论和观测应用研究，关注于活动星系核和黑洞双星的吸积过程。近年来也在开展星系团尺度弥散射电辐射的研究工作。

获奖及荣誉：

(2016年入会)

承担科研项目：

代表论著：

1-- Xie*, F. G., Yuan*, F., 2012, MNRAS, 427, 1580. Radiative efficiency of hot accretion flows

2-- Yang, Q. X., Xie*, F. G., Yuan*, F. et al., 2015, MNRAS, 447, 1692. Correlation between the photon index and X-ray luminosity of black hole X-ray binaries and active galactic nuclei: observations and interpretation

3-- Xie*, F. G., Yuan*, F., Ho, L. C., 2017, ApJ, 844, 42. Radiative Heating in the Kinetic Mode of AGN Feedback.

4-- Xie*, F. G., Yuan*, F., 2016, MNRAS, 456, 4377. Interpreting the radio/X-ray correlation of black hole binaries based on the accretion-jet model

5-- Yan*, Z., Xie*, F. G., Zhang, W., 2020, ApJL, 889, L18. Coronal Properties of Black Hole X-ray Binaries in the Hard State as Seen by NuSTAR and Swift

代表性论文（英文）：

1-- Xie*, F. G., Yuan*, F., 2012, MNRAS, 427, 1580. Radiative efficiency of hot accretion flows

2-- Yang, Q. X., Xie*, F. G., Yuan*, F. et al., 2015, MNRAS, 447, 1692. Correlation between the photon index and X-ray luminosity of black hole X-ray binaries and active galactic nuclei: observations and interpretation

3-- Xie*, F. G., Yuan*, F., Ho, L. C., 2017, ApJ, 844, 42. Radiative Heating in the Kinetic Mode of AGN Feedback.

4-- Xie*, F. G., Yuan*, F., 2016, MNRAS, 456, 4377. Interpreting the radio/X-ray correlation of black hole binaries based on the accretion-jet model

5-- Yan*, Z., Xie*, F. G., Zhang, W., 2020, ApJL, 889, L18. Coronal Properties of Black Hole X-ray Binaries in the Hard State as Seen by NuSTAR and Swift

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