@phdthesis{Kukulus2004,
  author    = {Kukulus, Matthias},
  title     = {A quantitative approach to the evolution of the central Walvis Basin offshore NW-Namibia : structure, mass balancing, and hydrocarbon potential},
  url       = {http://nbn-resolving.de/urn:nbn:de:bvb:20-opus-11075},
  school      = {Universit{\"a}t W{\"u}rzburg},
  year      = {2004},
  abstract  = {Rifting and breakup of Westgondwana in the Late Jurassic/ Early Cretaceous initiated the formation of the South Atlantic and its conjugated pair of passive continental margins. The Walvis Basin offshore NW-Namibia is an Early Cretaceous to recent depositional centre with a typically wedge-shaped postrift sedimentary succession covering an area of 105000km2. A 2D model transect across the central Walvis Basin and adjacent onshore areas is used as a case study to investigate quantitatively the denudational history of the evolving passive margin and the related contemporaneous depositional postrift evolution offshore. The database for both the onshore and offshore part of the model traverse is well constrained by own field work, published data as well as by seismic and well data supported by samples. The ultimate goal of this project is to present an integrated approach towards a quantitative link between surface processes and internal processes in terms of a mass and process balance.},
  subject      = {Namibia <Nordwest>},
  language  = {en}
}
@phdthesis{Berndt2002,
  author    = {Berndt, Roman},
  title     = {Palaeoecology and taxonomy of the macrobenthic fauna from the Upper Cretaceous Ajlun Group, southern Jordan},
  url       = {http://nbn-resolving.de/urn:nbn:de:bvb:20-opus-10974},
  school      = {Universit{\"a}t W{\"u}rzburg},
  year      = {2002},
  abstract  = {The Upper Cretaceous Ajlun Group (Cenomanian-Turonian) of southern/south-eastern Jordan has been analysed in 15 detailed sections with thicknesses between 40 m and 200 m. Taxonomic, palaeoecological, taphonomic, and sedimentological aspects were taken into account. During the early Upper Cretaceous the study area was situated at the south-eastern margin of the Tethys Ocean, between the palaeo-shoreline in the south-east and an offshore carbonate platform in the west. Thus, the measured sections include a complete facies succession from terrestrial-dominated environments via marginal marine siliciclastics to an area of carbonate precipitation. So far, very little is known about the fauna and the depositional environment of the group, especially of the transitional marginal marine part. Also, in depth studies of the Cretaceous fauna of southern Jordan are very rare. Therefore, the benthic fauna of the area is described in an extensive taxonomic chapter. It consists of 117 taxa, 77 of which are bivalves, 22 gastropods, 9 echinoids, and 4 corals. The phyla Porifera, Bryozoa, and Brachiopoda are represented by 1 species each. Additionally, at least two species of decapod crustaceans were found. One bivalve species is new: Anthonya jordanica from Cenomanian claystones of the eastern study area. 41 quantitative samples of the benthic invertebrate fauna were grouped into nine associations and three assemblages by means of a Q-mode cluster analysis. These are described as remnants of former communities and their environments are discussed. Salinity and substrate consistency are assumed to have been the most important environmental parameters controlling the faunal distribution. The overall palaeo-environment is discussed on the basis of sedimentological and palaeoecological results. It was primarily influenced by the morphology of the sea floor, sediment supply, and salinity of the sea water.},
  subject      = {Ajlun <Region>},
  language  = {en}
}
@phdthesis{Brandt2003,
  author    = {Brandt, S{\"o}nke},
  title     = {Metamorphic evolution of ultrahigh-temperature granulite facies and upper amphibolite facies rocks of the Epupa Complex, NW Namibia},
  url       = {http://nbn-resolving.de/urn:nbn:de:bvb:20-opus-10930},
  school      = {Universit{\"a}t W{\"u}rzburg},
  year      = {2003},
  abstract  = {The high-grade metamorphic Epupa Complex (EC) of north-western Namibia constitutes the south-western margin of the Archean to Proterozoic Congo Craton. The north-eastern portion of the EC has been geochemically and petrologically investigated in order to reconstruct its tectono-metamorphic evolution. Two distinct metamorphic units have been recognized, which are separated by ductile shear zones: (1) Upper amphibolite facies rocks (Orue Unit) and (2) ultrahigh-temperature (UHT) granulite facies rocks (Epembe Unit). The rocks of the EC are transsected by a large anorthosite massif, the Kunene Intrusive Complex (KIC). The Orue Unit and the Epembe Unit were affected by two distinct Mesoproterozoic metamorphic events, as is evident from differences in their metamorphic grade, in the P-T paths and in the age of peak-metamorphism: (1) The Orue Unit consists of a Palaeoproterozoic volcano-sedimentary sequence, which was intruded by large masses of I-type granitoids and by rare mafic dykes. During the Mesoproterozoic (1390-1318 Ma) the Orue Unit rocks underwent upper amphibolite facies metamorphism. The volcano-sedimentary sequence is constituted by interlayered basaltic amphibolites and rhyolitic felsic gneisses, with intercalations of migmatitic metagreywackes, migmatitic metapelites, metaarkoses and calc-silicate rocks. The Orue Unit was subdivided into three parts, which record similar heating-cooling paths but represent individual crustal levels: Heating led to the partial replacement of amphibole, biotite and muscovite through dehydration melting reactions. The peak-metamorphic P-T conditions of c. 700°C, 6.5 +/- 1.0 kbar (south-eastern part), c. 820°C, 8 +/- 0.5 kbar (south-western part) and c. 800°C, 6.0 +/- 1.0 kbar (northern part) correlate well with the mineral assemblage in the metapelites, i.e. Grt-Bt-Sil gneisses and schist in the south-eastern and south-western region and (Grt-)Crd-Bt gneisses in the northern part. Peak-metamorphism was followed by retrograde cooling to middle amphibolite facies conditions. Contact metamorphism, related with the intrusion of the anorthosites, is restricted to the direct contact to the KIC and recorded by massive metapelitic Grt-Sil-Crd felses, formed under upper amphibolite facies conditions (c. 750°C, c. 6.5 kbar). (2) The Epembe Unit consists of a Palaeoproterozoic volcano-sedimentary succession, which was intruded by small bodies of S-type granitoids and by andesitic dykes. All these rocks underwent UHT granulite facies metamorphism during the early Mesoproterozoic (1520-1447 Ma). The volcano-sedimentary succession is dominated by interlayered basaltic two-pyroxene granulites and rhyolitic felsic granulites. Migmatitic metapelites and metagreywackes are intercalated in the metavolcanites. Sapphirine-bearing MgAl-rich gneisses occur as restitic schlieren in the migmatitic metagreywackes. Reconstructed anti-clockwise P-T paths are subdivided into several distinct stages: During prograde near-isobaric heating to UHT conditions at c. 7 kbar biotite- or hornblende-bearing mineral assemblages were almost completely replaced by anhydrous mineral assemblages through various dehydration melting reactions. A subsequent pressure increase of 2-3 kbar led to the formation of the peak-metamorphic mineral assemblages Grt-Opx and (Grt-)Opx-Cpx in the orthogneisses and Grt-Opx, Grt-Sil and (Grt-)(Spr-)Opx-Sil-Qtz in the paragneisses. UHT-Metamorphism is proved by conventional geothermobarometry (970 +/- 70°C; 9.5 +/- 2.5 kbar), by the very high Al content of peak-metamorphic orthopyroxene (up to 11.9 wt.\% Al2O3) in many paragneisses and by Opx-Sil-Qtz assemblages in the MgAl-rich gneisses. Post-peak decompression is recorded by several corona and symplectite textures, formed at the expense of the peak-metamorphic phases: Initial UHT decompression of about ca. 2 kbar to 940 +/- 60°C at 8 +/- 2 kbar is mainly evident from the formation of sapphirine-bearing symplectites in the Opx-Sil gneisses. Subsequent high-temperature decompression to 6 +/- 2 kbar at 800 +/- 60°C resulted in the formation of Crd-Opx-Spl, Crd-Opx and Spl-Crd symplectites. Subsequent near-isobaric cooling to upper amphibolite conditions of 660 +/- 30°C at 5 +/- 1.5 kbar led to the re-growth of biotite, hornblende, sillimanite and garnet. During continued decompression orthopyroxene and cordierite were formed at the expense of biotite in several paragneisses. In a geodynamic model UHT metamorphism of the Epembe Unit is correlated with the formation of a large magma chamber at the mantle-crust boundary, which forms the source for the anorthosites of the KIC. In contrast, amphibolite facies metamorphism of the Orue Unit is ascribed to a regional contact metamorphic event, caused by the emplacement of the anorthositic crystal mushes in the middle crust.},
  subject      = {Namibia <Nordwest>},
  language  = {en}
}
@phdthesis{Schoell2003,
  author    = {Sch{\"o}ll, Achim},
  title     = {High-resolution investigation of the electronic structure of organic thin films},
  url       = {http://nbn-resolving.de/urn:nbn:de:bvb:20-opus-10809},
  school      = {Universit{\"a}t W{\"u}rzburg},
  year      = {2003},
  abstract  = {Die vorliegende Arbeit befasst sich mit der elektronischen Struktur organischer D{\"u}nnfilme. Eine zentrale Frage dabei ist der Einfluss der Wechselwirkung zwischen den Molek{\"u}len in der kondensierten Phase und der Wechselwirkung an metall-organischen Grenzfl{\"a}chen auf die elektronischen Eigenschaften. Dazu wurden die experimentellen Methoden Photoelektronenspektroskopie (PES) und R{\"o}ntgenabsorptionsspektroskopie (NEXAFS) mit h{\"o}chster Energieaufl{\"o}sung angewandt. Zus{\"a}tzlich wurden ab initio Rechnungen zur theoretischen Simulation von NEXAFS Spektren durchgef{\"u}hrt. Haupts{\"a}chlich wurden d{\"u}nne, vakuumsublimierte Filme aromatischer Modellmolek{\"u}le mit sauerstoffhaltigen funktionellen Gruppen (NTCDA, PTCDA, NDCA, BPDCA und ANQ) auf Ag(111) Oberfl{\"a}chen untersucht. Die ausgew{\"a}hlten Molek{\"u}le besitzen wegen ihrer großen delokalisierten p-Elektronensysteme sehr interessante Eigenschaften f{\"u}r die Anwendung in elektronischen Bauelementen. Dank der hohen Energieaufl{\"o}sung von Synchrotronstrahlungsquellen der dritten Generation war es erstmals m{\"o}glich, die Schwingungsfeinstruktur in den NEXAFS Spektren dieser kondensierten großen Molek{\"u}le sichtbar zu machen. Der Vergleich der Daten verschiedener Molek{\"u}le liefert dabei interessante Einblicke in den Kopplungmechanismus zwischen dem elektronischen {\"U}bergang und der Schwingungsanregung. Obwohl die Molek{\"u}le eine Vielzahl verschiedener Schwingungsmoden besitzen, kann man in deren NEXAFS Spektren beobachten, dass die elektronischen {\"U}berg{\"a}nge jeweils an haupts{\"a}chlich eine Schwingungsmode koppeln. Die hochaufgel{\"o}sten XPS Spektren der Molek{\"u}le NTCDA, PTCDA, NDCA, BPDCA und ANQ zeigen bestimmte systematische Unterschiede, so dass diese Spektren als Fingerabdruck f{\"u}r die jeweilige Substanz verwendet werden k{\"o}nnen. Durch die vergleichende Auswertung der Spektren konnten die 1s Bindungsenergien aller chemisch unterschiedlichen Kohlenstoff- und Sauerstoffatome bestimmt werden. Zus{\"a}tzliche Strukturen in den Spektren k{\"o}nnen shake-up Satelliten zugeschrieben werden. Die f{\"u}nf Molek{\"u}le stellen ein ideales Modellsystem dar, um fundamentale Aspekte der Rumpfelektronenspektroskopie zu untersuchen, wie Anfangs- und Endzustandseffekte und Satelliten, die durch die intramolekulare und intermolekulare Elektronendichteverteilung im Grund- und rumpfionisierten Zustand beeinflusst werden. Ein wichtiger Punkt dieser Dissertation sind spektroskopische Untersuchungen strukturell unterschiedlicher NTCDA Monolagenphasen auf Ag(111), deren Existenz aus vorangegangenen Arbeiten bekannt ist. Deutliche Unterschiede in der elektronischen Struktur der verschiedenen Phasen, die auf die Metall-Adsorbat Wechselwirkung zur{\"u}ckzuf{\"u}hren sind, konnten sowohl mittels XPS als auch mittels NEXAFS aufgezeigt werden. Sowohl f{\"u}r die komprimierte also auch f{\"u}r die relaxierte NTCDA Monolage kann die Bindung ans Substrat als schwach chemisorptiv charakterisiert werden, was eindeutig aus der Analyse der Satellitenstrukturen in den O 1s und C 1s XPS Spektren hervorgeht, die durch die dynamische Abschirmung durch Ladungstransfer vom Substrat erzeugt werden. Die NEXAFS Daten zeigen konsistent eine teilweise Besetzung des NTCDA LUMOs. Sowohl f{\"u}r die komprimierte als auch f{\"u}r die relaxierte NTCDA Monolage finden hochinteressante Phasen{\"u}berg{\"a}nge in ungeordnete Tieftemperaturphasen beim Abk{\"u}hlen auf 160 K statt. Dabei wird die Adsorbat-Substrat Wechselwirkung st{\"a}rker und das LUMO wird vollst{\"a}ndig besetzt. Dies kann in den NEXAFS Spektren anhand des Verschwindens der zugh{\"o}rigen {\"U}berg{\"a}nge beobachtet werden. Die XPS Spektren zeigen gleichzeitig eine deutliche Abnahme der Intensit{\"a}t schlecht abgeschirmter Photoemissionszust{\"a}nde, was auf die nun effektivere Ladungstransferabschirmung zur{\"u}ckzuf{\"u}hren ist. F{\"u}r den Phasen{\"u}bergang der relaxierten Monolage konnte mittels temperaturabh{\"a}ngiger NEXAFS Messungen eindeutig ein Hystereseverhalten gezeigt und die Hysteresekurve bestimmt werden. Die Hysterese betr{\"a}gt etwa 20 K. Des weiteren wurde aus SPA-LEED Messungen die Aktivierungsenergie f{\"u}r den Phasen{\"u}bergang der relaxierten Monolage beim Abk{\"u}hlen auf ca. 60 meV bestimmt. Schließlich wurden NEXAFS Untersuchungen an Poly{\"a}thylenproben mit verschiedenem Komonomergehalt durchgef{\"u}hrt. Unterschiede in den Absorptionsspektren von Proben mit unterschiedlichem Komonomeranteil konnten eindeutig auf die unterschiedliche Kristallinit{\"a}t der Proben zur{\"u}ckgef{\"u}hrt werden, indem eine hochkristalline Probe in situ bis zur Schmelztemperatur geheizt wurde. Ab initio Rechnungen an einer Modelmatrix aus Butanmolek{\"u}len zeigen, dass die Spektren von kristallinem und amorphem Poly{\"a}thylen aufgrund der intermolekularen Wechselwirkung deutliche Unterschiede haupts{\"a}chlich f{\"u}r Resonanzen mit starkem Rydberg Charakter aufweisen. Damit lassen sich die Unterschiede in den Poly{\"a}thylenspektren durch die {\"U}berlagerung der Signaturen der kristallinen und amorphen Anteile erkl{\"a}ren, die je nach Kristallinit{\"a}t der Probe in unterschiedlichen Verh{\"a}ltnissen vorliegen.},
  subject      = {D{\"u}nne Schicht},
  language  = {en}
}
@phdthesis{Xiao2004,
  author    = {Xiao, Zheng},
  title     = {Blimp-1 Regulates Terminal Differentiation of T Cells},
  url       = {http://nbn-resolving.de/urn:nbn:de:bvb:20-opus-10530},
  school      = {Universit{\"a}t W{\"u}rzburg},
  year      = {2004},
  abstract  = {The transcriptional repressor-Blimp-1 terminates differentiation of B lymphocytes as well as myeloid cells. Our data show that Blimp-1 is highly expressed in freshly isolated murine primary T lymphocytes, particularly its minor splice variant. Ectopic expression of Blimp-1 by retroviral transduction neither dramatically altered secretion of IFN-{\~a} or IL-4 nor did it induce the ability to suppress as regulatory T cells. However, induction of Blimp-1 resulted in not only a significant reduction in the production of IL-2 but also an inability to proliferate as well as in the reduced viability. These results demonstrate that Blimp-1 might mark end stages of lineage differentiation in T cells.},
  language  = {en}
}
@phdthesis{Vukicevic2004,
  author    = {Vukicevic, Vladimir},
  title     = {Mechanisms of apoptosis modulation and their contribution to genomic instability in tumor cells},
  url       = {http://nbn-resolving.de/urn:nbn:de:bvb:20-opus-10605},
  school      = {Universit{\"a}t W{\"u}rzburg},
  year      = {2004},
  abstract  = {The concept of programmed cell death has been increasingly considered from various aspects since early 1970's. Primarily, knowledge of apoptosis referred to morphological changes in which chromatin is condensed and increasingly fragmented, revealed as small structure in the nucleus. The membrane shrinks and the cell becomes dense as can be seen by flow cytometry. Interestingly, similar modes of cell deletion were observed in nematodes indicating that apoptosis is a highly conserved machinery. Three Caeonorhabditis elegans gene products are found to have high homology with mammalian apoptotic genes: CED-9 inhibits apoptosis and is related to bcl-2; CED-3 and CED-4 promote apoptosis and are related to caspase 9 and APAF-1. Apoptosis is not accidental death, but a highly controlled and medically important molecular process. More general terms such as 'physiological' or 'regulated' cell death cover different morphologies and sequences. Programmed suicide of cells that were subjected to toxic exogenous and endogenous stimuli plays a key role in understanding cancer development and its treatment. Apoptosis involves sequences of events that may overlap and play contradictory or antagonistic roles in cell death. Generally, the ability to trigger apoptotic processes in cancer cells would benefit an organism by keeping homeostasis intact. Programmed cell death is a regularly present mechanism, for instance, in lymphocyte recruitment in the thymus where immature lymphocytes may recognize host antigens. Therefore, such lymphocytes become apoptotic and are removed by macrophages. Removal prevents possible autoimmune diseases. Unlike apoptosis, necrosis is a passive process of cell death recognizable by membrane morphological changes and accompanied by leakage of intracellular material into intercellular space that may cause inflammation in the organism. Signals that may initiate apoptosis are generally classified into two groups: signals that launch extrinsic apoptotic pathways starting with aggregation of death receptors and intrinsic apoptotic pathways starting with disruption of intracellular homeostasis such as the release of mitochondrial factors or DNA degradation. Early in the process, apoptotic signals may lead to a broad range of signaling mechanisms such as DNA repair and assessment of DNA damage (check points). Thus, failure in any of these steps can cause a defective apoptotic response that plays a decisive role in both tumorigenesis and drug resistance in tumor treatment. More distinctly, the capability of cancer cells to go into apoptosis prevents further neoplastic changes. Generally, the purpose of this study is to investigate the balance between formation of genomic damage and induction of apoptosis under genotoxic stress. After genotoxic insult there are different possibilities for the fate of a cell (Figure 1). The genomic integrity is analyzed at cellular checkpoints, usually leading to a delay in cell cycle progression if DNA was damaged. Mutations in genes such as p53 and p21 change the cellular response to genotoxic stress and may alter the balance between apoptosis and genomic damage. However, p53 is usually mutated or not expressed in 70\% of human tumors. Alterations in p53 states that reflect distinct apoptotic response upon induction of DNA damage were examined. In this study, three cell lines with distinct p53 states were used: TK6 harboring wild-type p53, WTK1 with mutated p53 and NH32 with knocked out p53. In the present work we applied different approaches to investigate the correlation between DNA damage and apoptotic responsiveness in cancer cell lines with different p53 states or in hormone responsive cell lines with over expressed bcl-2 gene. We were focused on effects caused by temporary down regulation of the p53 and Bcl-2 activity in human lymphoblastoid cell lines. In addition, we investigated the impact of estradiol-induced proliferation on apoptosis and DNA damage in stably transfected cells with bcl-2gene.},
  subject      = {Apoptosis},
  language  = {en}
}
@phdthesis{Mueck2004,
  author    = {M{\"u}ck, Alexander},
  title     = {The standard model in 5D : theoretical consistency and experimental constraints},
  url       = {http://nbn-resolving.de/urn:nbn:de:bvb:20-opus-10591},
  school      = {Universit{\"a}t W{\"u}rzburg},
  year      = {2004},
  abstract  = {The four-dimensional Minkowski space is known to be a good description for space-time down to the length scales probed by the latest high-energy experiments. Nevertheless, there is the viable and exciting possibility that additional space-time structure will be observable in the next generation of collider experiments. Hence, we discuss different extensions of the standard model of particle physics with an extra dimension at the TeV-scale. We assume that some of the gauge and Higgs bosons propagate in one additional spatial dimension, while matter fields are confined to a four-dimensional subspace, the usual Minkowski space. After compactification on an S^1/Z_2 orbifold, an effective four-dimensional theory is obtained where towers of Kaluza-Klein (KK) modes, in addition to the standard model fields, reflect the higher-dimensional structure of space-time. The models are elaborated from the 5D Lagrangian to the Feynman rules of the KK modes. Special attention is paid to an appropriate generalization of the Rxi-gauge and the interplay between spontaneous symmetry breaking and compactification. Confronting the observables in 5D standard model extensions with combined precision measurements at the Z-boson pole and the latest data from LEP2, we constrain the possible size R of the extra dimension experimentally. A multi-parameter fit of all relevant input parameters leads to bounds for the compactification scale M=1/R in the range 4-6 TeV at the 2 sigma confidence level and shows how the mass of the Higgs boson is correlated with the size of an extra dimension. Considering a future linear e+e- collider, we outline the discovery potential for an extra dimension using the proposed TESLA specifications as an example. As a consistency check for the various models, we analyze Ward identities and the gauge boson equivalence theorem in W-pair production and find that gauge symmetry is preserved by a complex interplay of the Kaluza-Klein modes. In this context, we point out the close analogy between the traditional Higgs mechanism and mass generation for gauge bosons via compactification. Beyond the tree-level, the higher-dimensional models studied extensively in the literature and in the first part of this thesis have to be extended. We modify the models by the inclusion of brane kinetic terms which are required as counter terms. Again, we derive the corresponding 4D theory for the KK towers paying special attention to gauge fixing and spontaneous symmetry breaking. Finally, the phenomenological implications of the new brane kinetic terms are investigated in detail.},
  subject      = {Standardmodell <Elementarteilchenphysik>},
  language  = {en}
}
@phdthesis{Murso2004,
  author    = {Murso, Alexander},
  title     = {Electronic response of phosphorus and nitrogen based ligands on metal coordination},
  url       = {http://nbn-resolving.de/urn:nbn:de:bvb:20-opus-10397},
  school      = {Universit{\"a}t W{\"u}rzburg},
  year      = {2004},
  abstract  = {Phosphorus and nitrogen containing ligands were examined in terms of their coordination flexibility. Combining these donor atoms of different hardness or softness in one molecule leads to the design of polyfunctional, ambidentate ligand systems with unique properties, because the different features associated with each donor atom confer unique reactivity to their metal complexes. The phosphane Ph2P(CH2Py) (Py = 2-pyridyl) is a very versatile starting material for the preparation of highly flexible, hemilabile, ambident ligands. C-deprotonation of this phosphane yields a Janus head, responding very sensitive to the Lewis-acidity and the charge concentration of the coordinated metal, adapting its coordination mode to the electronic requirements of the cation (electronic differentiation). Thus, bidentate (P,N)-chelating, tridentate (P,N)-chelating together with C-coordination and (C,N)-coordination is observed in the different metal complexes discussed in this work. Additionally, the oxidized derivative of the abovementioned phosphane, the iminophosphorane Ph2P(CH2Py)(NSiMe3), is discussed. The C-deprotonated anion of this iminophosphorane prefers (N,N')-side arm- rather than C-coordination. The electron deficient pyridyl substituent at the C-atom leads to charge delocalization in the anionic [Ph2P(CHPy)(NSiMe3]-moiety. The bonding parameters of the iminophosphorane and all its derivatives, together with the almost fixed 15N-NMR resonances for the imino nitrogen atoms in these compounds prove that hypervalent central phosphorus is not required to describe the bonding situation in iminophosphoranes.},
  subject      = {Phosphane},
  language  = {en}
}
@phdthesis{Dobrawa2004,
  author    = {Dobrawa, Rainer Anton},
  title     = {Synthesis and characterization of terpyridine-based fluorescent coordination polymers},
  url       = {http://nbn-resolving.de/urn:nbn:de:bvb:20-opus-10367},
  school      = {Universit{\"a}t W{\"u}rzburg},
  year      = {2004},
  abstract  = {Complexation properties of 2,2':6',2''-terpyridine (tpy) have been studied with a series of first row transition metal ions by UV-vis, 1H NMR and isothermal titration calorimetry and ƒ´H values for the tpy complexation processes have been determined. These studies reveal that Zn2+ is the best suited metal ion for the reversible coordination of the terpyridine ligand. Thus, supramolecular coordination polymerization of perylene bisimide fluorophores containing terpyridine functionalities have been investigated by using Zn2+ as metal ion. The formation of the dimeric complexes in the case of monotopic model comounds and coordination polymerization of ditopic functional building blocks have been confirmed by 1H NMR studies. The optical properties of dimeric and polymeric complexes have been investigated by UV-vis and fluorescence spectroscopy. The Zn2+ coordination to the terpyridine unit does not effect the advantageous fluorescence properties of perylene bisimide moieties. The reversibility of the formation of coordination polymers has been established by 1H NMR and additionally by DOSY NMR and fluorescence anisotropy measurements. Coordination polymer strands can be visualized by atomic force microscopy (AFM), which also reveals the formation of an ordered monolayer film at higher concentration. The average polymer length has been determined by AFM to 15 repeat units, which correlates well with the value estimated by 1H NMR to >10 repeat units.},
  subject      = {Terpyridinderivate <2},
  language  = {en}
}
@phdthesis{Nuernberger2004,
  author    = {N{\"u}rnberger, Dieter},
  title     = {The Galactic Starburst Region NGC 3603 : exciting new insights on the formation of high mass stars},
  url       = {http://nbn-resolving.de/urn:nbn:de:bvb:20-opus-10440},
  school      = {Universit{\"a}t W{\"u}rzburg},
  year      = {2004},
  abstract  = {One of the most fundamental, yet still unsolved problems in star formation research is addressed by the question "How do high mass stars form?". While most details related to the formation and early evolution of low mass stars are quite well understood today, the basic processes leading to the formation of high mass stars still remain a mystery. There is no doubt that low mass stars like our Sun form via accretion of gas and dust from their natal environment. With respect to the formation of high mass stars theorists currently discuss two possible scenarios controversely: First, similar to stars of lower masses, high mass stars form by continuous (time variable) accretion of large amounts of gas and dust through their circumstellar envelopes and/or disks. Second, high mass stars form by repeated collisions (coalescence) of protostars of lower masses. Both scenarios bear difficulties which impose strong constrains on the final mass of the young star. To find evidences for or against one of these two theoretical models is a challenging task for observers. First, sites of high mass star formation are much more distant than the nearby sites of low mass star formation. Second, high mass stars form and evolve much faster than low mass star. In particular, they contract to main sequence, hydrogen burning temperatures and densities on time scales which are much shorter than typical accretion time scales. Third, as a consequence of the previous point, young high mass stars are usually deeply embedded in their natal environment throughout their (short) pre-main sequence phase. Therefore, high mass protostars are rare, difficult to find and difficult to study. In my thesis I undertake a novel approach to search for and to characterize high mass protostars, by looking into a region where young high mass stars form in the violent neighbourhood of a cluster of early type main sequence stars. The presence of already evolved O type stars provides a wealth of energetic photons and powerful stellar winds which evaporate and disperse the surrounding interstellar medium, thus "lifting the courtains" around nearby young stars at a relatively early evolutionary stage. Such premises are given in the Galactic starburst region NGC 3603. Nevertheless, a large observational effort with different telescopes and instruments -- in particular, taking advantage of the high angular resolution and high sensitivity of near and mid IR instruments available at ESO -- was necessary to achieve the goals of my study. After a basic introduction on the topic of (high mass) star formation in Chapter 1, a short overview of the investigated region NGC 3603 and its importance for both galactic and extragalactic star formation studies is given in Chapter 2. Then, in Chapter 3, I report on a comprehensive investigation of the distribution and kinematics of the molecular gas and dust associated with the NGC 3603 region. In Chapter 4 I thoroughly address the radial extent of the NGC 3603 OB cluster and the spatial distribution of the cluster members. Together with deep Ks band imaging data, a detailed survey of NGC 3603 at mid IR wavelengths allows to search the neighbourhood of the cold molecular gas and dust for sources with intrinsic mid IR excess (Chapter 5). In Chapter 6 I characterize the most prominent sources of NGC 3603 IRS 9 and show that these sources are bona-fide candidates for high mass protostars. Finally, a concise summary as well as an outlook on future prospects in high mass star formation research is given in Chapter 7.},
  subject      = {Starburst-Galaxie},
  language  = {en}
}