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<!DOCTYPE HTML>
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<head>
<title>Prof. Feng Yuan | Black Hole Accretion and High Energy Astrophysics Group</title>
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<h1>Feng Yuan</h1>
<p>Vice Director of SHAO, and Director of Astrophysics Division</p>
</header>
<!-- Main -->
<div id="main">
<section id="introduction" class="main">
<div class="spotlight">
<section id="content" class="main">
<h2>Contact:</h2>
<p>80 Nandan Road, Shanghai, 200030, China<br/>Phone: +86-21-34775301<br/>Fax: +86-21-64384618<br/>Email: [email protected]</p>
<h2>Current Research interests:</h2>
<ul>
<li>Black hole accretion, jet, wind</li>
<li>AGNs feedback, galaxy evolution</li>
<li>Active galactic nuclei</li>
<li>Black hole X-ray binaries</li>
<li>Planet formation</li>
</ul>
<h2>Employment:</h2>
<ul>
<li>1997-1998: Lecturer, Physics Department, Nanjing Normal University</li>
<li>1998-2000: Postdoctoral Researcher, Astronomy Department, Nanjing University</li>
<li>2000-2002: Postdoctoral Researcher, Max-Planck Institute of Radio Astronomy, Germany</li>
<li>2002-2003: Postdoctoral Researcher, Center for Astrophysics, Harvard University, USA</li>
<li>2003-2005: Postdoctoral Researcher, Physics Department, Purdue University, USA</li>
<li>2005-present: Professor, Shanghai Astronomical Observatory, Chinese Academy of Sciences</li>
</ul>
<h2>Education:</h2>
<ul>
<li>1987-1991: B.Sc., Physics Department, Shandong University; Major: Theoretical Physics</li>
<li>1991-1994: M.Sc., Institute of Chemistry, Shandong University; Major: Quantum Chemistry</li>
<li>1994-1997: Ph.D., Center for Astrophysics, University of Science and Technology of China; Major: Astrophysics</li>
</ul>
<h2>Selected publications:</h2>
<ul>
<li>Yuan, F. Luminous hot accretion disks, 2001, MNRAS, 324, 119-127</li>
<li>Yuan, F., Quataert, E., & Narayan, R. Nonthermal Electrons in Radiatively Inefficient Accretion Flow Models of Sagittarius A*, 2003, ApJ, 598, 301-312</li>
<li>Yuan, F., Cui, W. The radio---X-ray correlation and quiescent state of black hole sources, 2005, ApJ, 629, 408-413</li>
<li>Yuan, F., Lin, J., Wu, K. & Ho, L. An MHD model for the formation of episodic jets, 2009, MNRAS, 395, 2183</li>
<li>Yuan, F., Bu, D., & Wu, M. Numerical Simulation of Hot Accretion Flows. II. Nature, Origin, and Properties of Outflows and their Possible Observational Applications, 2012, ApJ, 761,130</li>
<li>Wang, Q. et al. Dissecting X-ray-Emitting Gas Around the Center of Our Galaxy, 2013, Science, 341, 981</li>
<li>Yuan, F. & Narayan, R. Hot acretion flows around black holes, 2014, ARA&A, 52, 529</li>
<li>Yuan, F. Gan, Z., Narayan, R., Sadowski, A., Du, D. & Bai, X. Numerical Simulation of Hot Accretion Flows. III. Revisiting Wind Properties Using the Trajectory Approach, 2015, ApJ, 804, 101</li>
</ul>
<h2>Selected talks:</h2>
<ul>
<li><a href="./uploads/yuan_ppt/lhaf.ppt">Luminous hot accretion flows</a></li>
<li><a href="./uploads/yuan_ppt/SgrA.ppt">Accretion onto the supermassive black hole in our Galactic center</a></li>
<li><a href="./uploads/yuan_ppt/SGRA-LLAGN.ppt">Advection-dominated accretion: from Sgr A* to low-luminosity AGNs</a></li>
<li><a href="./uploads/yuan_ppt/CMEjet.ppt">An MHD model for episodic jets</a></li>
<li><a href="/uploads/yuan_ppt
/outflow.pptx">Numerical simu
lations of black hole accretion and outflow</a></li>
<li><a href="./uploads/yuan_ppt/agnfeedback.pdf">AGNs feedback in an elliptical galaxy</a></li>
</ul>
<p>Latest update: August 2016</p>
</section>
<span class="image right" style="margin-top: 0;margin-bottom: auto;"><img src="./author/feng-yuan/avatar.jpg" alt="" /><br/>See <a href="./uploads/CV&publication_YF.pdf">here</a> for a complete CV and list of publications<br/>Official <a href="http://sourcedb.shao.cas.cn/zw/zjrck/200906/t20090624_1802378.html">homepage</a> in SHAO<br/>Go to group <a href="index.html">homepage</a></span>
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<h2>Quick links</h2>
<ui>
<li style="list-style:none"><a href="index.html">Group Home</a></li>
<li style="list-style:none"><a href="feng-yuan.html">Prof. Feng Yuan</a></li>
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<li style="list-style:none"><a href="index.html/#member">Members</a></li>
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<section>
<h2>Related links</h2>
<ui>
<li style="list-style:none"><a href="http://astro-en.shao.cas.cn/" target="blank">Division of Astrophysics</a></li>
<li style="list-style:none"><a href="http://english.shao.cas.cn/" target="blank">Shanghai Astronomical Observatory</a></li>
<li style="list-style:none"><a href="http://english.cas.cn/" target="blank">Chinese Academy of Sciences</a></li>
</ui>
</section>
<section>
<h2>Contact</h2>
<ui>
<li style="list-style:none">Address: 80 Nandan Road, Shanghai 200030, China</li>
<li style="list-style:none">Tel: +86-21-64386191</li>
<li style="list-style:none">Email: [email protected]</li>
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<p class="copyright">© Black Hole Accretion and High Energy Astrophysics Group. All rights reserved.<br/>Latest update: August 2016</p>
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