• Home
  • About XAO
    • Brief Introduction
    • Directors
    • Organization
  • Research
    • Research Divisions
    • Observation Stations
    • Facilities
    • Laboratories
    • Annual Reports
  • Scientist
    • Professors
    • Associate Professors
  • Cooperation
  • Education
    • Graduate Education
    • Post-Doctor Fellow
    • Supervisors
  • QTT Project
  • Join Us
  • Research News
  • 中
  • Home
  • About XAO
    • Brief Introduction
    • Directors
    • Organization
  • Research
    • Research Divisions
    • Observation Stations
    • Facilities
    • Laboratories
    • Annual Reports
  • Scientist
    • Professors
    • Associate Professors
  • Cooperation
  • Education
    • Graduate Education
    • Post-Doctor Fellow
    • Supervisors
  • QTT Project
  • Join Us
  • HomeResearch News
  • Research News
    • Dec 20, 2019
      Seminar on Exchange and Cooperation between Beijing Normal University and Xinjiang Astronomical Observatory
      From 9-10 December 2019, the Beijing Normal University (BNU) and Xinjiang Astronomical Observatory (XAO) Cooperation and Exchange Seminar was held in Beijing. More than 40 scholars from both parties participated in this seminar.WANG Na, ...
    • Dec 13, 2019
      Variations in pulsar subpulse drift rate
      Unusual evolutionary features and complicated characteristics of drifting subpulses have been observed in some pulsars (Wright & Fowler 1981; Smits et al., 2005; Basu & Mitra 2018), described in terms of multiple subpulse drift rates, pr...
    • Dec 05, 2019
      Research Progress in the Energy Dissipation of Solar Wind Burst and Particles Acceleration of the Diffusive Shock
      Solar Eruption is the origin of the Solar Energetic Particles, and it is also the basic impact factor of the solar-terrestrial environment and the space weather. Coronal Mass Ejections (CME) driven-shock is considered to be the important...
    • Oct 11, 2019
      Effects of infall and outflow on massive star-forming regions
      Star formation begins with the collapse of dense clumps, and forms much more dense cores in its center. At the same time, outflow driven by the star formation activities in the dense core will take some materials away from the dense core...
    • Oct 11, 2019
      Spatial Variation of the Chemical Properties of Massive Star-forming Clumps
      Many authors have used molecular lines at millimeter such as N2H+(1–0), HCO+(1–0), HCN(1–0), HNC(1–0) an CN(1-0) to study the evolution of massive star forming regions, and try to find a chemical clock for massive star formation. How...
    • Oct 11, 2019
      Carbon isotope ratio in starburst galaxies
      Even though interstellar carbon isotope ratios are locally understood, in extragalactic space beyond the Magellanic Clouds they are almost unexplored. We lack information on objects outside the Local Group of galaxies tracing environment...
    First2122232425Last
    View More
    Copyright © Xinjiang Astronomical Observatory
    Address:150, Science 1-Street, Urumqi, Xinjiang 830011, China
    Tel:0991-3689373Fax:0991-3838628Email:zongheban@xao.ac.cn