name:谢富国
sex:男
shrz:
channel:专家人才库
pic:http://sourcedb.shao.cas.cn/zw/zjrck/201604/P020****.png
url:http://sourcedb.shao.cas.cn/zw/zjrck/201604/t**_**.json
xklb:天体物理
xl:博士研究生
dh:
zc:研究员
zw:
yzbm:200030
dzyj:fgxie@shao.ac.cn
txdz:上海市南丹路80号
grwy:个人主页：http://www.shao.ac.cn/fgxie
grjj:籍贯江苏，上海天文台“星系和宇宙学研究中心”副研究员，硕士生导师。2004<\/span>年于中国科学技术大学获理学学士，2009<\/span>年于上海天文台获理学博士学位。2009<\/span>年7<\/span>月至2011<\/span>年6<\/span>月在北京大学科维理天文与天体物理研究所）从事博士后研究工作。2009<\/span>年至今于上海天文台从事天体物理研究工作。<\/span>
主要研究领域为黑洞吸积及高能天体物理研究，主要关注低光度活动星系核及黑洞双星系统。<\/span><\/font><\/font><\/p>
hjjry:
dblz:　　摘选论文：<\/span><\/font><\/font><\/p>　　1, Xie F. G. & Yuan F., 2016, MNRAS, 456, 4377 Interpreting the radio\/X-ray correlation of black hole X-ray binaries based on the accretion-jet model<\/span><\/span><\/font><\/p>　　2, Yang Q. X., Xie F. G., Yuan F., Zdziarski A. A., Gierli<\/span>ń<\/span>ski M., Ho L. C., & Yu Z., 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<\/span><\/span><\/font><\/p>　　3, Xie F. G., Yang Q. X., & Ma R.,2014, MNRAS, 442, L110 Jet-dominated quiescent states in black hole X-ray binaries: the case of V404 Cyg<\/span><\/span><\/font><\/p>　　4, Ma R., Xie F. G., & Hou S., 2014, ApJ, 780, L14 Relationship between the Kinetic Power and Bolometric Luminosity of Jets: Limitation from Black Hole X-Ray Binaries, Active Galactic Nuclei, and Gamma-Ray Bursts<\/span><\/span><\/font><\/p>　　5, Nied<\/span>？<\/span>wiecki A., Xie F. G., & Stepnik A., 2013, MNRAS, 432, 1576 Gamma-ray emission from proton-proton interactions in hot accretion flows<\/span><\/span><\/font><\/p>　　6, Xie F. G. & Yuan F. 2012, MNRAS, 427, 1580 Radiative efficiency of hot accretion flows<\/span><\/span><\/font><\/p>　　7. Yuan F., Xie F., & Ostriker J. P., 2009, ApJ, 691, 98 Global Compton Heating and Cooling in Hot Accretion Flows<\/span><\/span><\/font><\/p>
cdkyxmqk:
yjfx:星系形成与演化<\/span>
xmen:Fuguo Xie
education:
at:Professor
add:80 Nandan Road, Shanghai 200030,P.R.China
dblz_en:　<\/font>摘选论文：<\/span><\/font><\/p>　　1, Xie F. G. & Yuan F., 2016, MNRAS, 456, 4377 Interpreting the radio\/X-ray correlation of black hole X-ray binaries based on the accretion-jet model<\/span><\/span><\/font><\/p>　　2, Yang Q. X., Xie F. G., Yuan F., Zdziarski A. A., Gierli<\/span>ń<\/span>ski M., Ho L. C., & Yu Z., 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<\/span><\/span><\/font><\/p>　　3, Xie F. G., Yang Q. X., & Ma R.,2014, MNRAS, 442, L110 Jet-dominated quiescent states in black hole X-ray binaries: the case of V404 Cyg<\/span><\/span><\/font><\/p>　　4, Ma R., Xie F. G., & Hou S., 2014, ApJ, 780, L14 Relationship between the Kinetic Power and Bolometric Luminosity of Jets: Limitation from Black Hole X-Ray Binaries, Active Galactic Nuclei, and Gamma-Ray Bursts<\/span><\/span><\/font><\/p>　　5, Nied<\/span>？<\/span>wiecki A., Xie F. G., & Stepnik A., 2013, MNRAS, 432, 1576 Gamma-ray emission from proton-proton interactions in hot accretion flows<\/span><\/span><\/font><\/p>　　6, Xie F. G. & Yuan F. 2012, MNRAS, 427, 1580 Radiative efficiency of hot accretion flows<\/span><\/span><\/font><\/p>　　7. Yuan F., Xie F., & Ostriker J. P., 2009, ApJ, 691, 98 Global Compton Heating and Cooling in Hot Accretion Flows<\/span><\/span><\/font><\/p>
jl_en: