Researchers from the Xinjiang Astronomical Observatory conducted a systematic study of the filamentary structure within the G53 molecular cloud. By combining multi-wavelength observations and simulations, they revealed for the first time that the filament is undergoing an "end-dominated collapse", a process that is driving star formation.
A research team led by Prof. LIANG Xu from the Hefei Institutes of Physical Science of the Chinese Academy of Sciences has developed an ultra-compact excimer laser roughly the size of a thermos bottle.
A research team led by the Shanghai Astronomical Observatory has used the Tianma Radio Telescope to conduct multi-band radio observations of the returning comet 12P/Pons-Brooks. They measured its water production rate during outburst activities and made the most distant detection of ammonia molecules in a Halley-type comet to date.
A research team led by Profs. WANG Mingtai and CHEN Chong from the Hefei Institutes of Physical Science has developed an antimony trisulfide solar cell with a record conversion efficiency of 8.21%. This achievement marks the highest performance ever reported for this type of solar cell.
Using high-resolution data from the one-meter New Vacuum Solar Telescope, a research team led by Prof. YAN Xiaoli from the Yunnan Observatories of the Chinese Academy of Sciences has conducted an in-depth study on the physical properties and oscillations of chromospheric fibrils surrounding a quiescent filament.
Researchers from the Xinjiang Astronomical Observatory have revealed the link between nulling fraction and emission height by simulating the examination of the correlations between radio pulse nulling fraction, emission height, and their emission geometry, offerring new insight into the inner workings of pulsar magnetospheres.
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