A research team from the Institute of Modern Physics has directly measured the masses of two highly unstable atomic nuclei, phosphorus-26 and sulfur-27. These precise measurements provide crucial information for determining the nuclear reaction rate during X-ray bursts, advancing our understanding of how elements are synthesized under such extreme conditions.
A research team from the Yunnan Observatories of the Chinese Academy of Sciences, in collaboration with other researchers, has developed a new method to estimate how stellar-mass compact objects (COs)—including black holes, neutron stars, and white dwarfs—accrete matter within active galactic nucleus (AGNs) disks. This work provides new insights into the evolution of these objects in extreme cosmic environments.
Using the Five-hundred-meter Aperture Spherical radio Telescope (FAST), Dr. WEN Zhigang from the Xinjiang Astronomical Observatory of the Chinese Academy of Sciences, together with collaborators, have unveiled the most detailed scintillation characteristics to date of the millisecond pulsar B1937+21.
A research team led by Prof. LIU Fanglin from the Hefei Institutes of Physical Science of the Chinese Academy of Sciences has developed a novel generative model-based method for ecological soundscape analysis.
A new study led by the Yunnan Observatories of the Chinese Academy of Sciences has detected quasi-periodic oscillation (QPO) signals in an unusual gamma-ray burst (GRB) event.
Using high-precision astrometry from the Gaia satellite and applying uniform, stringent selection criteria, researchers from the Xinjiang Astronomical Observatory have identified 400 candidate binary open clusters in the Milky Way; 268 of these were newly reported. The findings provide a unified, structured scheme for identifying and classifying galactic binary clusters.
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