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  • About XAO
    • Brief Introduction
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  • HomeResearch News
  • Research News
    • Jun 19, 2018
      The Interaction of Pulse Nulling and Subpulse Drifting
      Radio pulsars in the Milky Way Galaxy rotate rapidly and steadily, and their radiation beams rotate with the pulsars like beacons in the universe. Among the more than 2600 pulsars discovered so far, the radiation of some pulsars shows st...
    • May 25, 2018
      Research progress of the Galactic magnetar PSR J1745-2900
      Magnetars are commonly considered as rotating neutron stars whose inferred surface dipolar magnetic fields are extremely strong. Their X-ray and γ -ray luminosities are usually orders of magnitude larger than their spin-down luminosity....
    • Apr 28, 2018
      Successful Pass on the Inspection for the Construction of the Center for Astronomical Mega-Science, Chinese Academy of Sciences.doc
      In 2017, Chinese Academy of Sciences (CAS) carried out the acceptance test at the end of preparation phase for 12 institutes’ constructions of the four types of institutes in CAS. Based on the institute self-assessment, experts’ group ...
    • Apr 16, 2018
      ‘Research and Observation of Pulsar Rotation Instability’ Project of XAO Received the Award of the First Prize of the 2017 Xinjiang Autonomous Region Prize for Progress in Science and Technology
      Recently, the ‘Research and Observation of Pulsar Rotation Instability’ project of XAO was awarded the first prize of the 2017 Xinjiang Autonomous Region Prize for Progress in Science and Technology. Under the leadership of Dr. Na Wang...
    • Apr 08, 2018
      The Chief Designer of Mars Exploration Program visited XAO
      On 24 March 2018, the chief designer of the First Mars Exploration Program, together with his team, visited the Nanshan site of XAO and attended a mini-symposium with the leaders and researchers of XAO.During the symposium, Dr. Na Wang, ...
    • Apr 08, 2018
      Major progress for developing the dynamic Lane–Emden equation with radial inertial force and dynamic evolution model for prestellar molecular cloud cores
      Under the action of self-gravity, the initial conditions and hydrodynamic evolution of protostar formation inside molecular cloud cores are not yet fully explored; these are key problems to be solved in frontier astrophysics which also b...
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