A recent study by researchers from the Xinjiang Astronomical Observatory of the Chinese Academy of Sciences, in collaboration with the Shanghai Astronomical Observatory, Yunnan Observatories, and the University of Heidelberg, has identified four previously unknown primordial open cluster groups in the Milky Way.
An international team led by the National Astronomical Observatories has recently released new findings on dark energy detection. This discovery provides significant experimental support for the Quintom dark energy theory proposed by Prof. ZHANG Xinmin’s team from the Institute of High Energy Physics
A new study of diffuse dwarf galaxies is challenging the prevailing galaxy formation model within the standard Cold Dark Matter (CDM) framework, leading to a proposed new model of dark matter. Under the direction of Prof. WANG Huiyuan from the University of Science and Technology of China, the research team identified for the first time an exceptionally strong clustering pattern in diffuse dwarf galaxies.
An international team of researchers from the Shanghai Astronomical Observatory, the Kavli Institute for Astronomy and Astrophysics at Peking University, and the University of Cologne, has conducted the most sensitive, highest-resolution, and most complete survey to date of three representative molecular clouds in the Milky Way’s Central Molecular Zone.
Researchers led by Ph.D student Serikbek Sailanbek from the Xinjiang Astronomical Observatory of the Chinese Academy of Sciences has conducted a comprehensive analysis of dense star-forming clumps across the Milky Way using ammonia data obtained from the NanShan 26-m Radio Telescope.
A research team led by Prof. WANG Mingtai at the Hefei Institutes of Physical Science of the Chinese Academy of Sciences has developed a finely tuned method for growing titanium dioxide nanorod arrays with controllable spacing without changing individual rod size and demonstrated its application in high-performance solar cells.
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