A research team from the Hefei Institutes of Physical Science has constructed a copper (Cu) single-atom catalyst with a nitrogen-coordination structure. They used two-dimensional g-C3N4, derived from melamine pyrolysis, as a carrier to achieve efficient electrocatalytic urea synthesis under mild conditions.
Researchers from the Yunnan Observatories of the Chinese Academy of Sciences have unveiled a neural network-based automated method for identifying heartbeat stars—a rare type of binary star system.
A research team from the University of Chinese Academy of Sciences has revealed the failure mechanism of diamond under extreme electrical fields through in situ experiments and molecular dynamics simulations, providing critical insights for the design of robust diamond devices.
A research team from the Shanghai Astronomical Observatory (SHAO) of the Chinese Academy of Sciences has uncovered the origins of double-peaked narrow emission-line characteristics in galactic centers.
A joint research team from the Shanghai Astronomical Observatory and the University of Science and Technology of China used the Very Large Array to search for potential persistent radio emission from FRB 20250316A, one of the brightest non-repeating bursts ever detected.
Researchers from the Shanghai Astronomical Observatory have revealed for the first time how gas flows from vast distances toward the disk surrounding a nascent massive star in the process of star formation.
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