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  • HomeResearch News
  • Research News
    • Sep 30, 2018
      Dr. Yao Jumei from Xinjiang Astronomical Observatory Won the China Top Cited Author Award by IOP Publishing
      Dr. Yao Jumei, a researcher of Pulsar Group of Xinjiang Astronomical Observatory, won the China Top Cited Author Award by IOP Publishing at the end of August. The title of the academic paper is “A New Electron-density Model for Estimati...
    • Sep 25, 2018
      Research progress of the light variations in the high-amplitude delta Scuti star
      Based on the high precision time-series data from Kepler Space Telescope, Xinjiang Astronomical Observatory Optical Group Prof. Aili Esamuding et al. reported a weak modulation effect in a double-mode high-amplitude delta Scuti (HADS) st...
    • Sep 03, 2018
      The 7th Youth Astronomy Forum of the Chinese Astronomical Society was held in Urumqi
      The 7th Youth Astronomy Forum of the Chinese Astronomical Society was held in Urumqi, which hosted by Chinese Astronomical Society, Xinjiang Astronomical Observatory (XAO) and Xinjiang Branch of Youth Innovation Promotion Association of ...
    • Aug 07, 2018
      2018 Stars Clusters’ Symposium Held in Urumqi
      The 2018 Star Clusters’ Symposium hosted by the Xinjiang Astronomical Observatory was held in Urumqi during 1-7 July, 2018. More than 30 experts and graduate students participated in the meeting from National Astronomical Observatory, S...
    • 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....
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