Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China
Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai, 200030; and National Astronomical Observatoires, Chinese Academy of Sciences, Beijing 100012, China Astronomical Observatory, Chinese Academy of Sciences; National Astronomical Observatoires, Chinese Academy of Sciences
Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, China
Shanghai Observatory
Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, People's Republic of China; and National Astronomical Observatoires, Chinese Academy of Sciences, Beijing 100012, People's Republic of China
Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, P.R. China; Joint Institute for Galaxy and Cosmology, ShAO and USTC, CAS, P.R. China; Graduate School of Chinese Academy of Sciences, Beijing 100039, P.R. China Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China; Joint Institute for Galaxy and Cosmology, ShAO and USTC, Chinese Academy of Sciences, China
Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China ; Joint Institute for Galaxies and Cosmology, Shanghai Astronomical Observatory and University of Science and Technology of China, Chinese Academy of Sciences, Shanghai 200030, China
Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China; and National Astronomical Observatoires, Chinese Academy of Sciences, Beijing 100012, China
Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030; and National Astronomical Observatoires, Chinese Academy of Sciences, Beijing 100012, People's Republic of China
A possible plasma jet in Comet Hale-Bopp
Analysis of the light variation periods of NGC 4151.
Brightness temperature for 166 radio sources
CCD imaging of the fragment S of Comet SL9 during its collision with Jupiter
CCD imaging of the fragment S of comet SL9 during the collision with Jupiter.
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