SJ
Suoqing Ji
Fudan University, Shanghai Astronomical Observatory, University of California, Santa Barbara, California Institute of Technology
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Galaxies: Formation, Evolution, Phenomena · Astrophysics and Star Formation Studies · Astrophysical Phenomena and Observations
0000-0001-9658-0588
Employment
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Fudan University Associate Professor2024 - Present
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Shanghai Astronomical Observatory Associate Professor2021 - 2024
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California Institute of Technology Sherman Fairchild Fellow2018 - 2021
Education
- 2013 - 2018
Projects & Funding
Projects & funding information is unavailable.
Publications (38)
- The mass-dependent interplay of active galacitc nuclei and supernova feedback in shaping the LX–T relation of early-type galaxies Save
- Solving the cooling flow problem with combined jet-wind AGN feedback Save
- Positive AGN Feedback Enhances Star Formation in Starburst Dwarf Galaxies Save
- A Systematic Study of AGN Feedback in a Disk Galaxy Using MACER. II. Predictions of X-Ray Surface Brightness Profiles and Comparison with eROSITA Observations Save
- A Systematic Study of AGN Feedback in a Disk Galaxy. I. Global Overview Save
- The non-universal pseudo-phase-space density profiles of symphony host haloes Save
- Turbulence and Star Formation Suppression in Elliptical Galaxies: The Role of Active Galactic Nucleus Jet–Wind Interaction Save
- Active Galactic Nucleus Feedback in an Elliptical Galaxy. IV. The Importance of the Jet–Wind Coupling Save
- MACER3D—An Upgrade of MACER2D with Enhanced Subgrid Models and Gas Physics—and Its Application to Simulating AGN Feedback in a Massive Elliptical Galaxy Save
- FEASTS Combined with Interferometry. III. The Low Column Density H i Around M51 and Possibility of Turbulent-mixing Gas Accretion Save
- Observational Evidence for Hot Wind Impact on Parsec Scales in Low-luminosity Active Galactic Nuclei Save
- On the dominant role of wind in the quasar feedback mode in the late-stage evolution of massive elliptical galaxies Save
- A simple sub-grid model for cosmic ray effects on galactic scales Save
- Magnetohydrodynamic simulations of the Tayler instability in rotating stellar interiors Save
- Constraining cosmic ray transport with observations of the circumgalactic medium Save
- Radiative turbulent mixing layers at high Mach numbers Save
- Standard self-confinement and extrinsic turbulence models for cosmic ray transport are fundamentally incompatible with observations Save
- A reduced speed-of-light formulation of the magnetohydrodynamic-particle-in-cell method Save
- First predicted cosmic ray spectra, primary-to-secondary ratios, and ionization rates from MHD galaxy formation simulations Save
- Numerical study of cosmic ray confinement through dust resonant drag instabilities Save