Laboratoire d’Études du Rayonnement et de la Matière en Astrophysique et Atmosphères

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Soutenance de thèse de Binh PHAM

par Valerie Audon - publié le

J’ai le plaisir de vous inviter à ma soutenance de thèse, "Satellite remote sensing of the variability of the continental hydrology cycle in the lower Mekong basin over the last two decades",

qui se déroulera le Mardi 06 Février 2018 à 14:00 dans la salle Danjon, Observatoire de Paris et au pot qui suivra.

Cette thèse est co-encadrée par Catherine Prigent et Filipe Aires.


Séminaires à venir

Vendredi 17 janvier 2020, 14h00
Salle de l'atelier, Paris
The role of feedback- and accretion-driven turbulence in galaxy build-up
résumé :
Cosmological models describe accurately the growth of large scale, dark matter-dominated, structures, but largely fail to reproduce the baryon content and physical properties of galaxies. Why? Essentially because the build-up of galaxies is regulated by a complex interplay between gravitational collapse, galaxy merging and feedback related to AGN and star formation, for which we still miss a robust theory. The energy released by these processes has to dissipate for gas to cool, condense, and form stars. How gas cools is thus a key to understand galaxy formation and why it such an inefficient process. In this seminar, I will discuss a few examples where turbulence driven by gas accretion, feedback, and galaxy interactions, which is largely ignored in models of galaxy formation, and captured in current simulations only over a limited range of scales, may have a major impact on galaxy and halos properties.

Vendredi 24 janvier 2020, 14h00
Salle de l'atelier, Paris
The accretion-ejection connection in planet-forming disks. New perspectives from high angular resolution observations
Vendredi 7 février 2020, 14h00
Salle de l'atelier, Paris
Redistribution of angular momentum from core to disk scales in Class 0 stars
Mathilde GAUDEL
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