Search results You are only searching within this website. To find search results for other University of Bonn websites, such as those of the faculties or institutes, please use a search engine. 1170 items matching your search terms. Filter the results Item type Select All/None EasyForm Collection Template-Folder Fontfamily Medien-Ordner Person Register Link Language Root Folder News Icon Language Independent Folder Person Business Card Folder Image Subsite Tiles-Seite Person Business Card Reference Event VideourlCT File New items since Yesterday Last week Last month Ever Sort by relevance date (newest first) alphabetically Full Wolfgang Paul lecture hall for the Physics Colloquium by Grant Sanderson Located in News / Bonn Physics Colloquium: Where Physics and Math collide Grant Sanderson with the organisers of the Physics Colloquium Located in News / Bonn Physics Colloquium: Where Physics and Math collide Grant Sanderson in the Bonn Physics Colloquium Located in News / Bonn Physics Colloquium: Where Physics and Math collide Prof. Dr. Carsten Urbach - from the Helmholtz-Institute for Radiation and Nuclear Physics at the University of Bonn is spokesperson for the new Collaborative Research Center "NuMeriQS: Numerical Methods for Dynamics and Structure Formation in Quantum Systems". Located in News / New Collaborative Research Center at the University of Bonn Christmas Physics Show 2023 Located in News / Christmas Physics Show 2023 View of the ring-laser lab Located in News / Inauguration of the ring laser gyroscopes This X-ray image shows the full extent of the Virgo Cluster, - which is the closest galaxy cluster (collection of galaxies) to us. The bright white spot at the center is the central galaxy M87 (known for the picture of the supermassive blackhole as observed by the Event Horizon Telescope). The hazy white glow around M87 is the very hot gas between galaxies. It extends out more in some directions than others, and isn’t circular; this is evidence that the Virgo Cluster is still in the process of forming. The colourful stripe in the bottom left comes from foreground emission inside our own galaxy and is known as one of the eROSITA bubbles. Located in News / eROSITA: The X-ray sky opens to the world eROSITA X-ray image with the newly discovered filament between two galaxy clusters. - The distribution of galaxies (white contours), as seen from the Two Micron All Sky Survey, follows the structure of the filament. In the SLOW simulation, which is tailored to reproduce the main features of the Local Universe, this individual system with both clusters and the filament spine is reproduced as well. Located in News / eROSITA: The X-ray sky opens to the world Virgo Located in News / eROSITA: The X-ray sky opens to the world Two new cluster initiatives at the University of Bonn - are given the green light to apply for funding as part of the Excellence Initiative of the German government and federal states Located in News / Major Success for University of Bonn < Previous 10 items 1 ... 27 28 29 30 31 32 33 ... 117 Next 10 items > UniID Please fill out this field using the example format provided in the placeholder. The phone number will be handled in accordance with GDPR.