Mapping the conditions for hydrodynamic instability on steady-state accretion models of protoplanetary disks T Pfeil, H Klahr The Astrophysical Journal 871 (2), 150, 2019 | 67 | 2019 |
The Sandwich Mode for Vertical Shear Instability in Protoplanetary Disks T Pfeil, H Klahr The Astrophysical Journal 915 (2), 130, 2021 | 36 | 2021 |
Handbook of Exoplanets H Klahr, T Pfeil, A Schreiber, HJ Deeg, JA Belmonte Springer, 2018 | 26 | 2018 |
High-resolution parameter study of the vertical shear instability–II: dependence on temperature gradient and cooling time N Manger, T Pfeil, H Klahr Monthly Notices of the Royal Astronomical Society 508 (4), 5402-5409, 2021 | 25 | 2021 |
Instabilities and flow structures in protoplanetary disks: Setting the stage for planetesimal formation H Klahr, T Pfeil, A Schreiber arXiv preprint arXiv:1806.03896, 2018 | 21 | 2018 |
Pseudo-riemannian VSI spaces II S Hervik Classical and Quantum Gravity 29 (9), 095011, 2012 | 20 | 2012 |
Dust Coagulation Reconciles Protoplanetary Disk Observations with the Vertical Shear Instability. I. Dust Coagulation and the VSI Dead Zone T Pfeil, T Birnstiel, H Klahr The Astrophysical Journal 959 (2), 121, 2023 | 12 | 2023 |
A Neural Network Subgrid Model of the Early Stages of Planet Formation T Pfeil, M Cranmer, S Ho, PJ Armitage, T Birnstiel, H Klahr arXiv preprint arXiv:2211.04160, 2022 | 2 | 2022 |
TriPoD: Tri-Population size distributions for Dust evolution-Coagulation in vertically integrated hydrodynamic simulations of protoplanetary disks T Pfeil, T Birnstiel, H Klahr Astronomy & Astrophysics 691, A45, 2024 | | 2024 |
Vertical shear instability with dust evolution and consistent cooling times. On the importance of the initial dust distribution T Pfeil, T Birnstiel, H Klahr arXiv preprint arXiv:2406.10335, 2024 | | 2024 |
Modeling Dust Evolution in Hydrodynamic Simulations of Protoplanetary Disks: New Methods and Applications T Pfeil Universitätsbibliothek der Ludwig-Maximilians-Universität, 2024 | | 2024 |