An international research team led by Dr. CUI Lang from the Xinjiang Astronomical Observatory has imaged the compact weak radio emission region and measured the astrometric parameters with high precision for the radio star AR Scorpii.
Researchers led by Dr. SHI Xiangdong and Prof. QIAN Shengbang from Yunnan Observatories have detected a total of 155 massive pulsating stars or candidates based on TESS, LAMOST and Gaia data.
According to a recent study, a collaborative research team from the Hefei Institutes of Physical Science and the University of Science and Technology of China has developed a research platform to study superconducting magnetic detection and magnetic phase transitions of hydrides under high pressure.
A research group led by Prof. LIU Changsong from the Hefei Institutes of Physical Science has developed a set of software to simulate the evolution of displacement damage in polycrystalline metals at over time and space scales, which was named object kinetic Monte Carlo-lattice kinetic Monte Carlo hybridization simulation software.
A research team led by Prof. LUO Xuan from Hefei Institutes of Physical Science made a breakthrough in tunning electronic properties of Weyl semimetal Td-MoTe2 by intercalating 3d-element Fe atoms into the van der Waals gap.
Researchers led by Dr. YANG Yong and Dr. ZHAO Jingkun from the National Astronomical Observatories have discovered a new stellar stream from dwarf galaxy in the Milky Way. This finding will enlarge the stream number originated from dwarf galaxy.
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