TALKS |
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2024 |
Waterloo Centre for Astrophysics |
What sets the vertical structure of the Milky Way's disk? |
2024 |
Shanghai, Conference |
The Gaia Snail and the Iron Snail: Leearning from Our Diverse Galactic Backyard |
2024 |
AIP, Potsdam |
What sets the vertical structure of the Milky Way's disk? |
2024 |
Ringberg meeting, dynamics workshop |
Iron Snails: non-equilibrium dynamics and spiral abundance patterns |
2024 |
AAS Madison Wisconsin |
Star Scattering in the MW: Evidence from Abundances & Streaming Motions |
2024 |
AIP, Potsdam |
What sets the structure of the LMC? |
2024 |
ISTA, Klosterneuburg, Austria |
Seeing the Milky Way Disk Evolve |
2023 |
Queen's University, Kingston |
What sets the vertical structure of the Milky Way's disk? |
2023 |
IAS Princeton |
Measuring the evolution of the Milky Way disk in real time |
2023 |
Bovy Group Meeting |
What sets the structure of the LMC? It depends on [M/H] |
2022 |
MPIA Group Meeting |
What gas Gaia DR3 done for us? Collecting Zebras in Phase Space |
2022 |
KITP Group Meeting |
The Gaia Snail and the Gaia Zebra |
2022 |
Bovy Group Meeting |
What Sets the Vertical Structure of Disk Galaxies in TNG50 Simulations? |
2021 |
Bovy Group Meeting |
Learning From Galactic Bars in Cosmological Simulations |
2021 |
EAS meeting |
Milky Way Analogs in TNG50: (what) can we learn from the bar? |
2021 |
Strasbourg Observatory |
Fitting the Secular Evolution of the Milky Way's Disk |
2021 |
INAF, Laura Bassi series |
What Sets the Structure of the MW Disk? Insight from Gaia and TNG50 |
2021 |
Heidelberg, MPIA GCTheory |
What Sets the Structure of Bars in TNG50’s MW Analogs? |
2021 |
ECOGAL Meeting |
What Drives the Evolution of Simulated Milky Way-like Disks? |
2020 |
ESO Seminar |
Inferring the Dynamical Structure of the Galactic Disk |
2020 |
Barcelona, ICCUB Seminar |
Seeing the Galactic Disk Evolve |
2020 |
Harvard, CfA seminar |
Seeing the Galactic Disk Evolve |
2020 |
Heidelberg, Patzer Colloquium |
Keeping it Cool: Much Migration, yet Little Heating, in the MW Disk |
2020 |
Harvard GC Group Meeting |
What Sets the Radial Structure of the Milky Way's Disk? |
2020 |
EAS Meeting |
Measuring Radial Migration with APOGEE and Gaia |
2020 |
Aarhus, Stars Group meeting |
Seeing the Milky Way Disk Evolve with Red Clump Stars |
2020 |
Birmingham, Stars Group meeting |
What Sets the Radial Structure of the MW Disk? |
2020 |
Cambridge UK, Galaxies Seminar |
Seeing the Milky Way Disk Evolve |
2020 |
Cambridge UK, MW Group meeting |
Modelling the Disk: Dynamics, Chemistry and Supernovae |
2020 |
Heidelberg MPIA, Seminar |
The Dynamical Evolution of the MW Disk is Cool |
2019 |
Paris Observatory, GEPI Seminar |
Seeing the Milky Way Disk Evolve |
2019 |
Stuttgart, AG meeting |
Building a Global Model for the Secular Evolution of the MW disk |
2019 |
Lund, white board talk |
Evolution of Galaxy Disks: what the Milky Way can do for you |
2019 |
Kloster Schoental, MPIA retreat |
How to Make a Galaxy Disk in Three Steps: Application to the Milky Way |
2018 |
Shanghai, life and times of the MW |
Measuring Radial Orbit Migration in the Milky Way Disk |
2018 |
Besancon, APOGEE-2 team meeting |
Obtained Diret Measure of Radial Migration with APOGEE |
2018 |
Lund, Dynamics for All |
What Sets the Radial Structure of the Milky Way Disk? |
2018 |
Heidelberg MPIA, Seminar |
What Sets the Radial Structure of the Milky Way Disk? |