2 resultados para Non-gravitational force

em KUPS-Datenbank - Universität zu Köln - Kölner UniversitätsPublikationsServer


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Over the past decades star formation has been a very attractive field because knowledge of star formation leads to a better understanding of the formation of planets and thus of our solar system but also of the evolution of galaxies. Conditions leading to the formation of high-mass stars are still under investigation but an evolutionary scenario has been proposed: As a cold pre-stellar core collapses under gravitational force, the medium warms up until it reaches a temperature of 100 K and enters the hot molecular core (HMC) phase. The forming central proto-star accretes materials, increasing its mass and luminosity and eventually it becomes sufficiently evolved to emit UV photons which irradiate the surrounding environment forming a hyper compact (HC) and then a ultracompact (UC) HII region. At this stage, a very dense and very thin internal photon-dominated region (PDR) forms between the HII region and the molecular core. Information on the chemistry allows to trace the physical processes occurring in these different phases of star formation. Formation and destruction routes of molecules are influenced by the environment as reaction rates depend on the temperature and radiation field. Therefore, chemistry also allows the determination of the evolutionary stage of astrophysical objects through the use of chemical models including the time evolution of the temperature and radiation field. Because HMCs host a very rich chemistry with high abundances of complex organic molecules (COMs), several astrochemical models have been developed to study the gas phase chemistry as well as grain chemistry in these regions. In addition to HMCs models, models of PDRs have also been developed to study in particular photo-chemistry. So far, few studies have investigated internal PDRs and only in the presence of outflows cavities. Thus, these unique regions around HC/UCHII regions remain to be examined thoroughly. My PhD thesis focuses on the spatio-temporal chemical evolution in HC/UC HII regions with internal PDRs as well as in HMCs. The purpose of this study is first to understand the impact and effects of the radiation field, usually very strong in these regions, on the chemistry. Secondly, the goal is to study the emission of various tracers of HC/UCHII regions and compare it with HMCs models, where the UV radiation field does not impact the region as it is immediately attenuated by the medium. Ultimately we want to determine the age of a given region using chemistry in combination with radiative transfer.

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Tissue mechanics and cellular interactions influence every single cell in our bodies to drive morphogenesis. However, little is known about mechanisms by which cells sense physical forces and transduce them from the cytoskeleton to the nucleus to control gene expression and stem cell fate. We have identified a novel nuclear-mechanosensor complex, consisting of the nuclear membrane protein emerin (Emd), actin and non-muscle myosin IIA (NMIIA), that regulates transcription, chromatin remodeling and lineage commitment. Force-induced enrichment of Emd at the outer nuclear membrane leads to a compensation between H3K9me2,3 and H3K27me3 on constitutive heterochromatin. This strain-induced epigenetic switch is accompanied by the global rearrangement of chromatin. In parallel, forces promote local F-actin polymerization at the outer nuclear membrane, which limits the availability of nuclear G-actin. Subsequently, the reduction of nuclear G-actin results in attenuated global transcription and therefore increased H3K27me3 occupancy to reinforce gene silencing. Restoring nuclear actin levels in the presence of mechanical strain counteracts PRC2-mediated silencing of transcribed genes. This mechanosensory circuit is also observed in vivo. Depletion of NMIIA in mouse epidermis leads to decreased H3K27me3 levels and precocious lineage commitment, thus abrogating organ growth and patterning. Our results reveal how mechanical signals regulate nuclear architecture, chromatin organization and transcription to control cell fate decisions.