TB
Tilman Birnstiel
Ludwig-Maximilians-Universität München, Center for Astrophysics Harvard & Smithsonian, Heidelberg University, University at Albany, State University of New York, Max Planck Institute for Astronomy
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Astrophysics and Star Formation Studies · Stellar, planetary, and galactic studies · Astro and Planetary Science
0000-0002-1899-8783
Employment
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Ludwig-Maximilians-Universitat Munchen Professor2017 - Present
- 2015 - 2021
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Max-Planck-Institut für Astronomie Postdoctoral Researcher2015 - 2017
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Harvard-Smithsonian Center for Astrophysics Postdoctoral fellow2013 - 2015
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Universitäts-Sternwarte München LMU Postdoctoral researcher2011 - 2012
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Max-Planck-Institut für Astronomie Postdoctoral researcher2010 - 2011
Education
- 2007 - 2010
- 2006 - 2007
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Bayerische Julius-Maximilians-Universität Vordiplom and graduate studies2003 - 2006
Projects & Funding
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C2: Gone with the wind: dust entrainment in photoevaporative winds German Research Foundation2017 - Present
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Composition of planets with an N-body-Monte-Carlo approach German Research Foundation2017 - Present
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Pebble accretion and the composition of exoplanets German Research Foundation2017 - Present
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Identifying the origin of Earth's building material: Where do the earth building Planetesimals and Pebbles originate from? A numerical approach of the accretion phase of the earth. German Research Foundation2015 - Present
Publications (251)
- Late-infall-induced formation of giant planets, multigenerational planetesimals, and disk substructures Save
- Interpreting the scattering surface in protoplanetary disks Save
- Dust characterization of halos: The extended emission in protoplanetary disks Save
- Planet formation at the inner edge of the dead zone Save
- A tension between dust and gas radii: The role of substructures and external photoevaporation in protoplanetary disks Save
- Starlight-driven flared-staircase geometry in radiation hydrodynamic models of protoplanetary disks Save
- Modeling dust dynamics in OpenGadget3 Save
- Formation of Multiple Dynamical Classes in the Kuiper Belt via Disk Dissipation Save
- Turbulence Inhibits Planetesimal Formation in Class 0/I Disks Subject to Infall Save
- Turbulence Inhibits Early Planetesimal Formation Save
- Refractory carbon depletion by photolysis through dust collisions and vertical mixing Save
- Planetesimal formation in a pressure bump induced by infall Save
- Kinematical signatures: Distinguishing between warps and radial flows Save
- High-resolution ALMA Observations of Richly Structured Protoplanetary Disks in σ Orionis Save
- TriPoD: Tri-Population size distributions for Dust evolution Save
- A Dust-trapping Ring in the Planet-hosting Disk of Elias 2-24 Save
- Population synthesis models indicate a need for early and ubiquitous disk substructures Save
- Sequential giant planet formation initiated by disc substructure Save
- Sequential giant planet formation initiated by disc substructure Save
- Vertical shear instability with dust evolution and consistent cooling times Save