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Wenfei Yu

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80 Nandan Road, Shanghai
 Yu Wenfei received his Bachelor’s degree in Physics and Master’s degree in Theoretical Physics in the Department of Physics, Central China University in 1990 and 1993, respectively. In 1998 he obtained his Ph.D in Particle Physics in the Institute of High Energy Physics (IHEP) of the Chinese Academy of Sciences (CAS). He had worked in the Division of Particle Astrophysics of IHEP in 1994–2001 and visited the CGRO/BATSE group in Marshall Space Flight Center in 1996-1998. He also worked in the `Anton Pannekoek’ Institute for Astronomy of the University of Amsterdam and in the Department of Physics of the University of Illinois at Urban-Champaign in 2001-2006 before he joined Shanghai Astronomical Observatory (SHAO) in late 2006 through the CAS One Hundred Talents Program. His current interest is on X-ray timing, spectral and polarization probes of fundamental physics in black hole and neutron star X-ray binaries, and is engaging in developing a competitive group at SHAO with space and ground multi-wavelength observations of Galactic and extra-Galactic high energy transients.  


Selected Publications: 

 (1) Yu, W., Yang, L., Wu, X.1994. Stability of an Isothermal Magnetized Accretion Disc with Radial Viscous Force. Monthly Notices of the Royal Astronomical Society 270, 131.  (2) Zhang, S. N., Yu, W., Zhang, W. 1998. Spectral State Transitions in Aquila X-1: Evidence for ``Propeller'' Effects. The Astrophysical Journal 494, L71-L74.  

  (3) Yu, W., van der Klis, M., Jonker, P. G. 2001. Dependence of Kilohertz Quasi-periodic Oscillation Properties on the Normal-Branch Oscillation Phase in Scorpius X-1.  The Astrophysical Journal 559, L29-L32.  

  (4) Yu, W., van der Klis, M.  2002. Kilohertz Quasi-periodic Oscillation Frequency Anticorrelated with Millihertz Quasi-periodic Oscillation Flux in 4U 1608-52. The Astrophysical Journal 567, L67-L70.  

  (5) Yu, W., Klein-Wolt, M., Fender, R., van der Klis, M. 2003. Hard X-Ray Flares Preceding Soft X-Ray Outbursts in Aquila X-1: A Link between Neutron Star and Black Hole State Transitions. The Astrophysical Journal 589, L33-L36.  

  (6) Yu, W., Lamb, F.K., Fender, R., van der Klis, M. 2007. Peak Luminosities of the Hard States of GX 339-4: Implications for the Accretion Geometry, Disk Mass, and Black Hole Mass. The Astrophysical Journal 663, 1309-1314.  

  (7) Yu, W., Dolence, J. 2007. A Hard-to-Soft State Transition during a Luminosity Decline of Aquila X-1. The Astrophysical Journal 667, 1043-1047.  

  (8) Yu, W., Yan, Z. 2009. State Transitions in Bright Galactic X-ray Binaries: Luminosities Span by Two Orders of Magnitude. The Astrophysical Journal 701, 1940-1957.  

  (9) Wu, Y. X., Yu, W., Li, T.P., Maccarone, T.J., Li, X. D. 2010. Orbital Period and Outburst Luminosity of Transient Low Mass X-ray Binaries. The Astrophysical Journal 718, 620-631.  

  (10) Yan, Z., Yu, W. 2012. An ultraviolet flux drop preceding the X-ray hard-to-soft state transition during the 2010 outburst of GX 339-4. Monthly Notices of the Royal Astronomical Society 427, L11-L15.  

  (11) Yu, W., Zhang, W. 2013 Energy-dependent Power Spectral States and Origin of Aperiodic Variability in Black Hole Binaries.\ The Astrophysical Journal 770, 135.  

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