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.
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.
Researchers from the Yunnan Observatories have discovered that the orbital evolution of the supersoft X-ray source WX Centauri (WX Cen) is dominated by the angular momentum loss (AML) driven by magnetic wind from the donor secondary and from the accretion disk alone or together.
Dr. SHAN Hao from Xinjiang Astronomical Observatory and his collaborators carried out a preliminary study on the high dynamic range radio source detection algorithm based on the full set alternative data release 1of TIFR GMRT Sky Survey.
Researchers from the Yunnan Observatories and the Max Planck Institute reanalyzed properties of extremely eccentric planetary system HD 76920b through detailed asteroseismic analysis of its host star HD 76920.
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