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  • About XAO
    • Brief Introduction
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  • HomeResearch News
  • Research News
    • Apr 25, 2024
      Researchers Observe Emission Lines in Planck Cold Cores with Nanshan 26-m Radio Telescope
      Recently , Dilda Berdikhan , a PhD student from the star formation and evolution research group of the Xinjiang Astronomical Observatory ( XAO ) of the Chinese Academy of Sciences ( CAS ) ., emission lines , with 187 cores detected hyper...
    • Apr 24, 2024
      Improving timing precision of millisecond pulsars using polarization
      Used data obtained from the Five-hundred-meter Aperture Spherical Radio Telescope ( FAST ) to carry out a study of white noise in MSPs . The study was published in The Astrophysical Journal . The researchers presented measurements of the...
    • Apr 19, 2024
      Pulsars with non-stopping pulsed emission
      Radio pulsars are well known for their regular pulses .The researchers from Xinjiang Astronomical Observatory ( XAO ) of the Chinese Academy of Sciences ( CAS ) used simulation to investigate the properties of the non-nulling pulsars .Co...
    • Mar 21, 2024
      XAO NanShan 26-m Radio Telescope Successfully Ran 4-Gbps VLBI Test Observations
      The Very Long Baseline Interferometry ( VLBI ) operation team at the Nanshan Station of Xinjiang Astronomical Observatory( XAO ) has recently got the NanShan 26 - meter Radio Telescope ( NSRT ) to participate in 4 - Gbps VLBI observation...
    • Mar 21, 2024
      Researchers have made progress studying the carbon-rich AGB star IRC+10216 (CW Leo) at 3mm band
      IRC+10216 (CW Leo) is the closest and the brightest carbon-rich (C /O > 1) asymptotic giant branch (AGB) star. Astronomers have detected 106 different species (not including isotopologues) in its circumstellar envelope (CSE), making this...
    • Mar 21, 2024
      Study highlights impact of C/O ratio on sulfur depletion in TMC-1
      It is crucial to estimate the elemental depletion in the interstellar medium ( ISM ) to successfully and accurately simulate the chemical evolution in various astrophysical environments such as molecular clouds or star forming regions .U...
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