Physics – Condensed Matter – Superconductivity
Scientist
Physics
Condensed Matter
Superconductivity
Scientist
National Observatories, Beijing, China
Beijing Astronomical Observatory, CAS; National Astronomical Observatories, CAS
National Astronomical Observatoires, Chinese Academy of Sciences, Beijing 100012, PR China
National Astronomical Observatoires, Chinese Academy of Sciences, Beijing 100012, China
National Astronomical Observatories, Chinese Academy of Sciences, 100012, Beijing, PR China
Institut für Astronomie und Astrophysik der Universität München, Scheinerstrasse 1, 81679 München, Germany; National Astronomical Observatoires, Chinese Academy of Sciences, Beijing 100012, PR China
Institute for Space Astrophysics, Department of Applied Physics, Shanghai Jiaotong University, Shanghai 200030, P.R.China
Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100012, P.R. China; Institute for Space Astrophysics, Department of Applied Physics, Shanghai Jiao Tong University, Shanghai 200030, P.R. China
National Astronomical Observatoires, Chinese Academy of Sciences, Beijing 100012, PR China; Chinese Academy of Sciences - Peking University Joint Beijing Astrophysical Center, Beijing 100871, PR China
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
Institut für Astronomie und Astrophysik der Universität München, Scheinerstrasse 1, 81679 München, Germany; National Astronomical Observatoires, Chinese Academy of Sciences, Beijing 100012, China
National Astronomical Observatoires, Chinese Academy of Sciences, Beijing 100012, PR China ; Institut für Astronomie und Astrophysik der Universität München, Scheinerstrasse 1, 81679 München, Germany
National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100012, PR China ; Universitäts-Sternwarte München, Scheinerstrasse 1, 81679, München, Germany
Institut für Astronomie und Astrophysik der Universität München, Scheinerstr. 1, 81679 München, Germany; National Astronomical Observatoires, Chinese Academy of Sciences, Beijing 100012, PR China
National Astronomical Observatoires, CAS,
A non-LTE study of neutral and singly-ionized iron line spectra in 1D models of the Sun and selected late-type stars
Abundances of Na, Mg and Al in nearby metal-poor stars
Abundances of nearby red clump giants (Liu+, 2007)
An analysis of the X-ray emission in the late stage of SN 1987 A
Atomic data of Zn I for the investigation of element abundances
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