Background: © ESO/José Francisco Salgado

About

  • since 2017

    Professor at LMU

    Since February 2017 I am a professor for theoretical astrophysics at the LMU Munich, leading an ERC funded research group on planet formation.

  • 2015-2016

    Postdoc at MPIA

    Moving back to Germany, I worked as a postdoc with Hubert Klahr and Thomas Henning at the MPIA in Heidelberg for 1.5 years.

  • 2013-2015

    Postdoc at CfA

    I spent almost 3 years at the Harvard-Smithsonian Center for Astrophysics in Cambridge, MA working with Sean Andrews and up to today keep an affiliation with the CfA as Research Associate for ongoing projects and collaborations.

  • 2011-2012

    Postdoc at LMU

    I was postdoctoral researcher at the LMU Munich and the Excellence Cluster 'Universe' working with Barbara Ercolano.

  • 2007-2010

    PhD in Astronomy

    I got my PhD in Astronomy from the University of Heidelberg, working at the Max-Planck-Institute of Astronomy under the supervision of Kees Dullemond. Afterwards I stayed at the MPIA as a postdoc until June 2011.

  • 2003-2007

    Studies at U. of Würzburg and State Univ. of New York

    I did my undergraduate studies at the University of Würzburg, Germany and my Masters at the State University of New York at Albany.

Research


The general topic of my research is the formation of planets as well as the structure and evolution of protoplanetary disks, the birthplaces of planets. More specifically, I am woking on the dynamics of solid particles in these disks and how they grow towards planets.

Young stars and the disks around them are built up from interstellar matter which contains only very small, at most micrometer-sized dust particles. This small dust is the material out of which planets form. However the mechanisms which lead to the growth along over 45 orders of magnitude in mass are still poorly understood. The aim of my work is to understand how grains can grow from small to large and how they are distributed and transported in the disk.

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These results have a vast impact on planet formation, disk structure and evolution and the chemistry of protoplanetary disks. I also work together with observers in order to compare my models to observational data and thus test the theory behind them. The questions we set out to answer are the following:

  • What causes the sub-structures we observe in disks? Do the disks already host planets or is something else shaping their appearance?
  • How can we use observations to probe the structure and evolution of protoplanetary disks?
  • Can our models help us understand features of our own solar system, such as the size distribution of chondrules found in meteorites, the isotopic composition of water, or the size of the solar system?
  • How can we explain the existence of mm-sized pebbles in the outer regions of disks? How do they form and how do they migrate?
  • When and where do the building blocks of planets emerge and what is their composition? Can we understand this with models based on current laboratory experiments?
  • What is the size and structure of so-called dead zones, i.e., regions where the disk is predicted to be non-turbulent and what is the role of fine dust grains in this picture?

Stats

The current stats according to NASA ADS are:

Refereed papers:
Citations:

You can download my CV or see all publications on ADS by clicking the buttons below.

Materials

Here you can download stills and animations of dust evolution simulations, latex templates, protoplanetary disk schematics. You can also find links to my codes and my Master's and PhD theses.


Research Group

Members

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Dr.
Joanna
Drążkowska
Postdoc

Working on coagulation in hydrodynamical simulations, on planetesimal formation, and on circumplanetary disks.

Homepage
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Dr.
Sebastian
Stammler
Postdoc

Working on dustpy (global dust evolution model), planetesimal formation, and pebble accretion.

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Fabian
Binkert
PhD Student

Working on vertical and radial transport of solids with particle histories.

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Apostolos
Zormpas
PhD Student

Working on disk population synthesis and physical modeling of disk emission profiles.

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Matías
Gárate
PhD Student

Working on Dust-Gas backreactions and effects of high dust-to-gas ratios.

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Anirudh
Sharma
Master's Student

Working on radiative transfer modeling and the dust content in IM Lup.

Funding

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Ludwig-Maximilians-Universität München

LMU hosts the group and provides base funding and a PhD position.


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European Research Council

The ERC project DustPrints (1.4 Million Euro) currently funds two postdocs and one PhD of the group.


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Deutsche Forscher Gemeinschaft

The DFG (German Science Foundation) funds parts of the group through the Origins Cluster and collaborations through the RUTD.

Teaching

Current Semester

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Essentials of Advanced Astrophysics (SS20) Lecture (Masters)
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Astrophysik des Sonnensystems (SS20) Seminar (Bachelor)

Previous Semesters

Press & Outreach

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Local
Media

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20 Ring Worlds
seen with
ALMA
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Planet Hunting
with
ALMA
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Most Detailed
Image of
a Disk
Image
A Dust
Clump
in HL Tau?
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A Frozen
Flying
Saucer
Image
Disk Gaps
Don't Always
Signal Planets
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Inner dust ring
around star
gets supplies abroad
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Popular
Science
Article
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Lucky
Dust
Particles
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Dust Trap
in IRS 48

Contact

Scheinerstr. 1, 81679 Munich, Germany

+49 (0) 89 2180 6973

til [dot] birnstiel [at] lmu [dot] de

© 2020 Til Birnstiel