简介: |
Galaxies are ecosystems of gas and stars, and we should ask about their connection in studying every aspect of galaxy evolution. While the development of HI (the atomic gas) science for galaxies is relatively lagged compared to other bands, we are in front of a golden age for it. I will present a series of my studies on cold gas accretion, star formation, star formation quenching and structure (morphology) evolution in galaxies based on a multi-wavelength and HI-involved observational method. I will also show the current limitations that can be overcome with the new radio facilities including the FAST telescope in the near future.
Bio: Dr. Jing Wang obtained her Phd for astrophysics from USTC (China) in Dec. 2011. She is currently a postdoc at Australia Telescope National Facility. She worked in Max-Planck Institute for Astrophysics (Germany) from 2008-2014, first as a visiting student and later as a postdoc, before moving to Australia. Her research has been focused on the evolution of galaxies, and based on a multi-wavelength observational method. |
