Séminaires

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18 février 2020

The LEGA-C Spectroscopic Survey of z ~ 1 Galaxies

Le 24 mars 2017 De 10h30 à 12h00 Arjen van der Wel MPIA Heidelberg We have precise constraints on the evolution of the cosmic stellar mass density and how stars are distributed over galaxies with different masses, sizes and morphologies. The next challenge is to decipher the...

18 février 2020

Superfluid Dark Matter

Le 17 mars 2017 De 10h30 à 12h00 Lasha Berezhiani Princeton I will talk about a novel theory of dark matter superfluidity that matches the success of LCDM model on cosmological scales while simultaneously reproducing the MOND phenomenology on galactic...

18 février 2020

Structure, dynamics and chemodynamics of the inner Galaxy

Le 24 février 2017 De 10h30 à 12h00 Matthieu Portail MPE Garching The Milky Way is a Rosetta stone for understanding how massive disk galaxies form and evolve. It is currently the subject of an extraordinary observational effort, providing data on a star-by-star basis for...

18 février 2020

Formation of local spiral galaxies

Le 17 février 2017 De 10h30 à 12h00 Myriam Rodrigues Observatoire de Paris In the Λ-CDM paradigm, the Universe is structured at large scales by the hierarchical assembly of dark matter haloes. To be a coherent framework, this cosmological model has to predict the evolution...

18 février 2020

The Acceleration Scale in Galaxy Dynamics

Le 10 février 2017 De 10h30 à 12h00 Stacy McGaugh Case Western There exists an empirical scale in galaxy dynamics connecting baryons with kinematics. The mass discrepancy appears at a particular acceleration scale, and grows progressively more severe at lower accelerations....

18 février 2020

Of pulsars and their winds

Le 16 décembre 2016 De 10h30 à 12h00 Bronislaw Rudak Nicolaus Copernicus Astronomical Center Neutron stars are important tools used in physics, astronomy and even cosmology. Our knowledge of these objects is based mostly on the studies of pulsars and associated phenomena...