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edoc.ub.uni-muenchen.de 檢索結果共 11226 筆,本頁資料從第 205 筆到第 216 筆

This thesis presents a study of the galaxy populations in massive galaxy clusters that have been selected via the Sunyaev - Zeldovich Effect from the South Pole Telescope. The clusters have multiband optical imaging data from the Dark Energy Survey (DES). Each cluster has a robust mass estimate and with the deep DES data they cover a redshift range between 0 and 1.1. Th....

By Christina Hennig--Ludwig-Maximilians-Universität München--2015-07-14
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By Anna Antipova--Ludwig-Maximilians-Universität München--2015-07-14
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In recent years there has been a considerable focus on the development of subunit vaccines, preferred over traditional vaccines for reasons of safety and purity. However, subunit vaccines are less immunogenic than attenuated vaccines and need therefor multiple administrations in combination with immunostimulatory adjuvants, in order to induce immunity. The sustained rel....

By Marie-Paule Even--Ludwig-Maximilians-Universität München--2015-07-14
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By Dominik Zgela--Ludwig-Maximilians-Universität München--2015-07-14
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The outer halos of galaxies are known to store vital information about the formation history and merger-induced evolution of their central galaxies, since the relaxation timescales are much larger than in the innermost parts and thus the memory of the events is conserved over a long period. This information provides fundamental insights into the processes of mass growth....

By Rhea-Silvia Remus--Ludwig-Maximilians-Universität München--2015-07-13
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By Lei Zhang--Ludwig-Maximilians-Universität München--2015-07-13
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The theory of Bishop spaces (TBS) is so far the least developed approach to constructive topology with points. Bishop introduced function spaces, here called Bishop spaces, in 1967, without really exploring them, and in 2012 Bridges revived the subject. In this Thesis we develop TBS. Instead of having a common space-structure on a set X and R, where R denotes the set o....

By Iosif Petrakis--Ludwig-Maximilians-Universität München--2015-07-13
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By Florian Karch--Ludwig-Maximilians-Universität München--2015-07-13
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Turbulence is one of the most widespread phenomena in nature occurring in fluids and plasmas at all scales - from the blood flow in the human body, via the Earth's atmosphere to the remnants of supernovas at astrophysical scales. Despite its frequent occurrence, constructing a theory of turbulent motion, which provides reliable quantitative predictions, represents o....

By Vasil Bratanov--Ludwig-Maximilians-Universität München--2015-07-10
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Diese Arbeit befasst sich mit der Entwicklung und dem Test optischer Frequenzkämme zur Kalibration astronomischer Spektrographen. Die Genauigkeit der besten Spektrographen war bisher durch ihre Kalibration begrenzt. Die Benutzung von Frequenzkämmen als hochgenaue optische Frequenzreferenz verspricht die Überwindung dieser Limitierung, und damit die Bestimmung von Lin....

By Rafael Probst--Ludwig-Maximilians-Universität München--2015-07-10
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By Johann Ahn--Ludwig-Maximilians-Universität München--2015-07-09
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Turbulence is a ubiquitous phenomenon in astrophysical plasmas. Most of these systems exhibit a property called cross helicity, a non-zero correlation between velocity fluctuations and magnetic-field fluctuations. In the presence of a magnetic mean-field, such as in the solar wind or in the interstellar medium, cross helicity is equivalent to an imbalance between Alfven....

By Martin S. Weidl--Ludwig-Maximilians-Universität München--2015-07-09
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