T. Birnstiel

Excellence Cluster Origins — Germany

Physics and Astronomy · Physical Sciences

45h-index9.1kcitations229works6.02yr avg
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Research Topics

Astrophysics and Star Formation Studies(169), Astro and Planetary Science(124), Stellar, planetary, and galactic studies(121), Molecular Spectroscopy and Structure(54), Astronomy and Astrophysical Research(21)

Publications229 total

Planet formation at the inner edge of the dead zone -- I: the interplay between accretion outbursts and dust growth
arXiv (Cornell University)·2026Open Access
Planet formation at the inner edge of the dead zone -- I: the interplay between accretion outbursts and dust growth
ArXiv.org·2026Open Access
A tension between dust and gas radii: the role of substructures and external photoevaporation in protoplanetary disks
arXiv (Cornell University)·2026Open Access
A tension between dust and gas radii: the role of substructures and external photoevaporation in protoplanetary disks
ArXiv.org·2026Open Access
Starlight-driven flared-staircase geometry in radiation hydrodynamic models of protoplanetary disks
Springer Link (Chiba Institute of Technology)·2026
Starlight-driven flared-staircase geometry in radiation hydrodynamic models of protoplanetary disks
Astronomy and Astrophysics·2026Open Access
General Implicit Runge–Kutta Integrators for Multifluid Gas–Dust Aerodynamic Drag
The Astrophysical Journal·2025Open Access
TriPoDPy: 1D Tri-Population size distributions forDust evolution in protoplanetary disks
arXiv (Cornell University)·2025Open Access
Formation of Multiple Dynamical Classes in the Kuiper Belt via Disk Dissipation
The Astrophysical Journal·2025· 1 citedOpen Access
General Implicit Runge-Kutta Integrators for Multifluid Gas-Dust Aerodynamic Drag
arXiv (Cornell University)·2025Open Access
Modeling dust dynamics in OpenGadget3
Astronomy and Astrophysics·2025Open Access
Modeling dust dynamics in OpenGadget3 -- I. SPH implementation of the One-Fluid model
arXiv (Cornell University)·2025Open Access
Detailed Microwave Continuum Spectra from Bright Protoplanetary Disks in Taurus
The Open Journal of Astrophysics·2025· 2 citedOpen Access
Turbulence Inhibits Planetesimal Formation in Class 0/I Disks Subject to Infall
The Astrophysical Journal·2025· 3 citedOpen Access
Turbulence Inhibits Early Planetesimal Formation
2025Open Access
Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): Evidence of planet–disk interaction in the 2MASSJ16120668-3010270 system
Astronomy and Astrophysics·2025· 4 citedOpen Access
Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): Evidence of planet-disk interaction in the 2MASSJ16120668-3010270 system
arXiv (Cornell University)·2025Open Access
Spirals, rings, and vortices shaped by shadows in protoplanetary discs: from radiative hydrodynamical simulations to observable signatures
Monthly Notices of the Royal Astronomical Society·2025· 9 citedOpen Access
Refractory carbon depletion by photolysis through dust collisions and vertical mixing
Astronomy and Astrophysics·2025· 5 citedOpen Access
Planetesimal formation in a pressure bump induced by infall
Springer Link (Chiba Institute of Technology)·2025
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Frequent Co-authors

Paola Pinilla(21), C. P. Dullemond(18), M. Benisty(12), Sean M. Andrews(10), C. Dominik(10), Andrea Isella(9), Luca Ricci(8), David J. Wilner(7), Laura M. Pérez(7), John M. Carpenter(6), Sebastian Markus Stammler(6), Zhaohuan Zhu(5), Karin I. Öberg(5), Jane Huang(5), A. Pohl(5), L. Testi(5), Th. Henning(5), E. F. van Dishoeck(4), Xue‐Ning Bai(4), Shangjia Zhang(4)