The research team led by Mao Yewei, faculty of the School of Physics and Materials Science of Guangzhou University(GU), analyzed the multi-band imaging data of far ultraviolet-near infrared observed by space and ground telescopes. They worked out the functional relationship of galaxy morphology with wavelength and the multi-band images of galactic nuclei and disks. The research paper entitled "Multi Wavelength Bulge–Disk Decomposition for the Galaxy M81 (NGC3031). i. Morphology" was published on The Astrophysical Journal Supplement Series, a internationally renowned astronomical journal.
The authors of the paper include Gong Junyu, a graduate student from the School of Physics and Materials Science, Mao Yewei who is the correspondent author, Gao Hua, a postdoctoral researcher at the University of Hawaii and Yu Siyue, a postdoctoral scholar at Humboldt Institute of Radio Astronomy in Germany. This research is supported by the National Natural Science Foundation of China (NSFC), Guangdong, Hong Kong and Macau Greater Bay Area Sub-center of the National Astronomical Science Data Center and the Peking University Keweili Institute of Astronomy and Astrophysics (PKU-KIAA).
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