Welcome to my homepage!@ Yellow Stone

I am a Postdoc Fellow at the Chile Observatory, National Astronomical Observatory of Japan, starting from August 1st, 2016. I received my PhD degree from Nanjing University, China, supervised by Prof. Qiusheng Gu and Dr. Qizhou Zhang, in June 2016. During 2012-2015 I also worked as an SMA Pre-doctoral Fellow at the Harvard-Smithsonian Center for Astrophysics, supervised by Dr. Qizhou Zhang.

My research focusses on high-mass star formation in massive molecular clouds throughout the Galaxy, from infrared dark clouds to the Central Molecular Zone. I use radio and sub-millimeter continuum and spectral line observations from e.g., the SMA, JVLA, GBT, IRAM 30m, and CSO, to study physical conditions in high-mass star formation regions from 1-pc to <0.1-pc scales.

I am also interested in programming to speed up our daily works. I use IDL and Python mostly (see below for a 3D scene of CO outflows I created with Python), while I am expericenced with Mathematica/Javascript.




National Astronomical Observatory of Japan
2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan


Click here to download a pdf version.

External links

My GitHub homepage
My Flickr Album
My Page on Astroleaks
Dr. Qizhou Zhang's Homepage
School of Astronomy & Space Science, Nanjing University

3D printed glass cube of G28.34
3D printed glass cube of CO outflows and dust emission in G28.34 as observed by ALMA.
(For the 3D model: Outflows in a massive star-forming cloud.)
(For the code to make such models: TDViz.)
(For the observational data: Zhang et al. 2015, ApJ, 804, 141.)