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I’m Feiyu Quan (全飞宇), a PhD student at The Chinese University of Hong Kong Star Formation Group studying astrophysics. Previously, I studied astrophysics at University of Toronto and University of Cambridge.

My research

Projection effects in observations

F. Quan et al., Projection Is All You Need: Interpreting Polarization Measurements in the Orion Clouds with Sub-Alfvénic MHD Simulations, submitted to ApJ.

Interactive visualizations of dense cores in molecular clouds and their surrounding magnetic fields (from the simulations in this work) can be found at here (misaligned magnetic fields) and here (aligned magnetic fields). (They could take a while to load. If they are not loading, clearing your browser’s cache might help.)

In these visualizations, the red field lines indicate that they pass through dense regions with volume density $ > 5 \times 10^4 \ {\rm H_2}\ \mathrm{cm}^{-3} $ , while the blue field lines pass through diffuse gas with volume density $ < 1 \times 10^4 \ {\rm H_2}\ \mathrm{cm}^{-3} $. The grey-scale color indicates different volume densities.

Compensating turbulence spectrum and zoom-in simulations of molecular clouds

Under construction…

Curriculum vitae

Click here to download my CV as a PDF file

Contact

Email: feiyu.quan@link.cuhk.edu.hk

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