Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Astronomical Institute, ``Anton Pannekoek'', University of Amsterdam
UIUC
Shanghai Astronomical Observatory
IHEP, China
Astronomical Institute "Anton Pannekoek", University of Amsterdam
University of Illinois at Urbana-Champaign
Shanghai Astronomical Observatory, Chinese Academy of Sciences
Shanghai Astronomical Observatory, China
University of Amsterdam, Kruislaan 403, 1098 SJ, Amsterdam, The Netherlands
Shanghai Astronomical Observatory, 80 Nandan Road, Shanghai 200030, China
LCRHEA, IHEP, Beijing
LCRHEA, IHEP, China
ES-84, NASA / Marshall Space Flight Center, Huntsville, AL, USA;
High Energy Astrophysics Lab., Institute of High Energy Physics;
University of Amsterdam
Institute of High Energy Physics, Academia Sinica, Beijing, China
University of Illinois
Laboratory for Cosmic Ray and High Energy Astrophysics, Institute of High Energy Physics, Beijing, China
Laboratory for Cosmic Ray and High Energy Astrophysics, Institute of High Energy Physics, Beijing 100039, China
High Energy Astrophysics Lab., Institute of High Energy Physics, P.O. Box 918-3, 100039, Beijing, China
High Energy Astrophysics Lab., Institute of High Energy Physics, P.O. BOX 918-3, 100039, Beijing, China
Astronomy Department, CAS-PKU Joint Beijing Astrophysics Center, Peking Univ., Beijing 100871, PR China; Institute of Inorganische Chemistry, Uni. Bonn, Roemer St., 53117 Bonn, Germany
UvA
Center for Theoretical Astrophysics, University of Illinois at Urbana-Champaign
Astronomical Institute, University of Amsterdam, Kruislaan 403, 1098 SJ, Amsterdam, The Netherlands
Shanghai Astronomical Observatory, 80 Nandan Road, Shanghai, China
LCRHEA, Institute of High Energy Physics, Beijing, 100039, China
75As NMR study of single crystals of the heavily overdoped pnictide superconductors Ba{1-x}KxFe2As2 (x = 0.7 and 1)
A Hard-to-Soft State Transition during A Luminosity Decline of Aquila X-1
A model for the waveform behavior of accreting millisecond pulsars: Nearly aligned magnetic fields and moving emission regions
A Model of Waveform Variations and Intermittency in Accretion-Powered Millisecond Pulsars
A UV flux drop preceding the X-ray hard-to-soft state transition during the 2010 outburst of GX 339-4
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