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  • HomeResearch News
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    • May 17, 2019
      Changes in spin-down rate and intermittent pulsars
      Suggests that sudden changes of some kind in pulsar magnetospheres are common .The growing number of pulsars with observed switching in emission properties suggests that sudden changes of some kind in pulsar magnetospheres are common. An extreme example is that found in intermittent pulsars whose emission exhibits ...
    • May 07, 2019
      XAO Wins 2018 Newcomb Cleveland Prize as a Member of Research Team of the Micius Quantum Satellite
      The research team of the Micius quantum satellite was awarded the 2018 Newcomb Cleveland Prize by the American Association for the Advancement of Science (AAAS) on February 2019, for the achievement of satellite-to-ground entanglement di...
    • Apr 16, 2019
      Research progress of the formaldehyde absorption line in Molecular Clouds
      The distribution of H2CO absorption in the Galaxy and against 262 Galactic radio sources has been surveyed showing that H2CO absorption is associated with most of the H II regions. Since H2CO is only seen in absorption against a backgrou...
    • Mar 06, 2019
      The structured jet was discovered in a binary neutron star merger
      The gravitational wave event GW170817 in August 2017 is the first binary neutron star merger event discovered so far, and its counterpart was detected in subsequent observations at almost all electromagnetic bands, which announced the a...
    • Jan 30, 2019
      The 4th International Youth Forum on Antenna Multidisciplinary Design and Measurement
      From 23-26 January, the “4th International Youth Forum on Antenna Multidisciplinary Design and Measurement” was held in Urumqi. Organized by Xinjiang Astronomical Observatory (XAO) and XiDian University, the forum focused on the theore...
    • Dec 12, 2018
      High-mass Outflows Identified from COHRS CO (3–2) Survey
      Molecular outflow is one of the significant and common features in star formation regions. The transition of angular momentum and radiation pressure makes star-forming continually proceeded and injects enough energy as turbulent energy o...
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