Pin-Gao Gu, Ph.D.
Affiliations: | 2000 | University of Texas at Austin, Austin, Texas, U.S.A. |
Area:
Astronomy and Astrophysics, Fluid and Plasma Physics, Radiation PhysicsGoogle:
"Pin-Gao Gu"Parents
Sign in to add mentor| Ethan T. Vishniac | grad student | 2000 | UT Austin | |
| (Turbulence in Keplerian accretion disks.) | ||||
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Publications
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| Gu P, Peng D, Yen C. (2019) Modeling the Thermal Bulge of a Hot Jupiter with the Two-stream Approximation The Astrophysical Journal. 887: 228 |
| Yen H, Gu P, Hirano N, et al. (2019) HL Tau Disk in HCO + (3─2) and (1─0) with ALMA: Gas Density, Temperature, Gap, and One-arm Spiral The Astrophysical Journal. 880: 69 |
| Yen H, Takakuwa S, Gu P, et al. (2019) Signs of outflow feedback from a nearby young stellar object on the protostellar envelope around HL Tauri Astronomy and Astrophysics. 623 |
| Tang Y, Guilloteau S, Dutrey A, et al. (2017) Planet Formation in AB Aurigae: Imaging of the Inner Gaseous Spirals Observed inside the Dust Cavity The Astrophysical Journal. 840: 32 |
| Yen HW, Liu HB, Gu PG, et al. (2016) GAS GAPS IN THE PROTOPLANETARY DISK AROUND THE YOUNG PROTOSTAR HL TAU Astrophysical Journal Letters. 820 |
| Wang H, Bu D, Shang H, et al. (2014) Formation of Isothermal Disks around Protoplanets. I. Introductory Three-dimensional Global Simulations for Sub-Neptune-mass protoplanets The Astrophysical Journal. 790: 32 |
| Hsieh H, Gu P. (2012) On The Secular Behavior Of Dust Particles In An Eccentric Protoplanetary Disk With An Embedded Massive Gas Giant Planet The Astrophysical Journal. 760: 119 |
| Chang YL, Bodenheimer PH, Gu PG. (2012) Coupled evolutions of the stellar obliquity, orbital distance, and planet'S radius due to the ohmic dissipation induced in a diamagnetic hot Jupiter around a magnetic T Tauri star Astrophysical Journal. 757 |
| Gu PG. (2010) Extrasolar planets: Larger than they ought to be. Nature. 465: 300-1 |
| Gu P, Ogilvie GI. (2009) Diurnal thermal tides in a non-synchronized hot Jupiter Monthly Notices of the Royal Astronomical Society. 395: 422-435 |