Seminare und Vorlesungen

The Milky Way in context

Biermann Lectures 2022: Insights on the Milky Way’s history and dynamics
All lectures take place in the MPA Large Seminar Room E.0.11 and will be preceded by tea, coffee and cookies at 15 minutes before the lecture starts. [mehr]

Revisiting disk demographics in the emerging paradigm of MHD disk winds

ESO Web Star and Planet Formation Seminar

Search for magnetized circumgalactic clouds using Faraday rotation

Cosmology Seminar

The first star clusters and SMBH formation therein

ORIGINS Mini Workshop

Comparing codes: a numerical (and human) adventure

ESO Informal Discussion - Hybrid

Towards robust cosmological inference from multi-wavelength galaxy cluster data

LMU Astrophysics Colloquium

Galactic Winds: From the Central Engine to the Circumgalactic Medium

MPA Special Seminar on Galaxy Formation
This review will summarize the latest results from multi-wavelengthstudies of gas and dust flows out of nearby and distantgalaxies. After a brief discussion of the basic physics and opentheoretical issues, I will present recent results on the origin ofwinds on sub-pc scales in nearby star-forming and activegalaxies. Next, I will describe multiphase galaxy-scale outflows indwarf galaxies and powerful quasars and their impact on the hostgalaxies. Finally, I will assess the latest observational evidence forgalactic winds reaching 100+ kpc scales out to the circumgalacticmedium. [mehr]

Galactic Winds: From the Central Engine to the Circumgalactic Medium

Special Seminar - Hybrid

Milky Way’s early history

Biermann Lectures 2022: Insights on the Milky Way’s history and dynamics
All lectures take place in the MPA Large Seminar Room E.0.11 and will be preceded by tea, coffee and cookies at 15 minutes before the lecture starts. [mehr]

Dynamics and the dark matter halo of the Milky Way

Biermann Lectures 2022: Insights on the Milky Way’s history and dynamics
All lectures take place in the MPA Large Seminar Room E.0.11 and will be preceded by tea, coffee and cookies at 15 minutes before the lecture starts. [mehr]

Going Non-Linear: Contrasting LCDM with the internal properties of galaxies

MPA Special Seminar on Galaxy Formation
The Lambda Cold Dark Matter (LCDM) paradigm has been spectacularly successful at reproducing observations of the cosmic microwave background and of the large scale structure of the Universe. On these scales, the structures contrasted with the theory are in the linear or mildly non-linear regime, where observations are well established and theoretical predictions are robust. LCDM also makes specific predictions in the non-linear regime; in particular, for the evolution, abundance, structure, and substructure of dark matter halos, the sites of galaxy formation. On these non-linear scales a number of potential challenges to LCDM have been identified when confronting the observed internal structure of galaxies with LCDM expectations. I plan to review briefly the status of these challenges and to discuss whether they signal a potential breakdown of the LCDM paradigm or just reflect our incomplete understanding of the complex process of galaxy formation. [mehr]

TBA

MPA Special Seminar on Galaxy Formation

TBA

MPA Special Seminar on Galaxy Formation
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