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    • 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...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...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.Curr...
    • Mar 07, 2024
      Researchers Discover a New Pulsar Possibly Associated with a Supernova Remnant
      Recently , a master ’ s student ZHANG Zhen supervised by Professor YAN Wenming from the pulsar research group of Xinjiang Astronomical Observatory , Chinese Academy of Sciences .Search results for the pulsar PSR J1845-0306 Contact : ZHA...Recently, a master’s student ZHANG Zhen supervised by Professor YAN Wenming from the pulsar research group of Xinjiang Astronomical Observatory, Chinese Academy of Sciences, used the Five-hundred-meter Aperture Spherical Radio Telescope...
    • Feb 02, 2024
      Researchers carry out H2CO observations of the Perseus molecular cloud using the NSRT telescope
      Recently, Umut Mahmut, a master’s student from the star formation and evolution research group of the Xinjiang Astronomical Observatory (XAO) of the Chinese Academy of Sciences (CAS), and his collaborators utilized the NanShan 26-meter ...Recently, Umut Mahmut, a master’s student from the star formation and evolution research group of the Xinjiang Astronomical Observatory (XAO) of the Chinese Academy of Sciences (CAS), and his collaborators utilized the NanShan 26-meter ...
    • Jan 25, 2024
      High resolution study reveals the radio nature of the magnetic propeller cataclysmic variable J0240+1952
      Using Very Long Baseline Interferometry ( VLBI ) observations .Researchers from the Xinjiang Astronomical Observatory ( XAO ) of the Chinese Academy of Sciences have imaged the compact radio emission region and detected radio flare event...Using Very Long Baseline Interferometry (VLBI) observations, researchers from the Xinjiang Astronomical Observatory (XAO) of the Chinese Academy of Sciences have imaged the compact radio emission region and detected radio flare events fo...
    • Jan 19, 2024
      Workshop on Pulsar and Nanohertz Gravitational Waves Detection Held at XAO
      The Workshop on Pulsar and Nanohertz Gravitational Waves Detection was successfully held at the Nanshan Station of Xinjiang Astronomical Observatory (XAO) from 15 to 17 January, organised by XAO. About 30 participants from Peking Univers...
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