Researchers from the Xinjiang Astronomical Observatory have conducted observational work on the SiC2 molecule in circumstellar envelopes of three carbon-rich AGB stars using the Atacama Large Millimeter/Submillimeter Array.
The nearby radio galaxy M87, located 55 million light-years from the Earth and harboring a black hole 6.5 billion times more massive than the Sun, exhibits an oscillating jet that swings up and down with an amplitude of about 10 degrees, confirming the black hole's spin.
A research group led by assistant professor WU Chengyuan from Yunnan Observatories has investigated the evolution of post-merger remnant resulting from the coalescence of double oxygen-neon white dwarfs.
Researchers from the Xinjiang Astronomical Observatory have found a hub filament system G323.46-0.08, which provides evidences for gravitational collapse and accretion flows.
Researchers from the Xinjiang Astronomical Observatory and their collaborators sorted out the multi-frequency observation data of repeating fast radio bursts, and studied the statistical characteristics of dispersion measure and the waiting time of FRB180916.J0158+65.
An international scientific team has revealed for the first time the magnetic field transport processes in the accretion flow of a black hole and the formation of a "MAD"—a magnetically arrested disk—in the vicinity of a black hole.
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