Modulation of host cell signaling pathways as a therapeutic approach in periodontal disease

Recently, new treatment approaches have been developed to target the host component of periodontal disease. This review aims at providing updated information on host-modulating therapies, focusing on treatment strategies for inhibiting signal transduction pathways involved in inflammation. Pharmacological inhibitors of MAPK, NFκB and JAK/STAT pathways are being developed to manage rheumatoid arthritis, periodontal disease and other inflammatory diseases. Through these agents, inflammatory mediators can be inhibited at cell signaling level, interfering on transcription factors activation and inflammatory gene expression. Although these drugs offer great potential to modulate host response, their main limitations are lack of specificity and developments of side effects. After overcoming these limitations, adjunctive host modulating drugs will provide new therapeutic strategies for periodontal treatment.

A theoretical study of the characterization and the absorption spectrum of Mg: Tetracycline complexes in aqueous environment.

The complex formed by the tetracycline (TC) molecule with the Mg ion is able to prevent the replication of the genetic material in the bacterial ribosome, making an excellent antibiotic. In general, the absorption and emission spectra of TC are very sensitive to the host ions and the pH of the solvent that the set is immersed. However, the theoretical absorption spectrum available in the literature is scarce and limited to simple models that do not consider the fluctuations of the liquid. Our aim is to obtain the electronic absorption spectrum of TC and the complex Mg:TC in the ratio 1:1 and 2:1. Moreover, we analyze the changes in intensity and shifts of the bands in the systems listed. We performed the simulation using the classical Monte Carlo technique with the Lennard-Jones plus Coulomb potential applied to each atom of the both TC molecule and the Mg:TC complexes in water. The electronic absorption spectrum was obtained from the time-dependent density functional theory using different solvent models. In general, we obtained a good qualitative description of the spectra when compared with the experimental results. The Mg atom shifts the first band by 4 nm in our models, in excellent agreement to the experimental result of 4 nm. The second absorption band is found here to be useful for the characterization of the position where the ion attaches to the TC.

Endotoxin exposure during sensitization to Blomia tropicalis allergens shifts TH2 immunity towards a TH17-mediated airway neutrophilic inflammation: role of TLR4 and TLR2

Experimental evidence and epidemiological studies indicate that exposure to endotoxin lipopolysaccharide (eLPS) or other TLR agonists prevent asthma. We have previously shown in the OVA-model of asthma that eLPS administration during alum-based allergen sensitization blocked the development of lung TH2 immune responses via MyD88 pathway and IL-12/IFN-γ axis. In the present work we determined the effect of eLPS exposure during sensitization to a natural airborne allergen extract derived from the house dust mite Blomia tropicalis (Bt). Mice were subcutaneously sensitized with Bt allergens co-adsorbed onto alum with or without eLPS and challenged twice intranasally with Bt. Cellular and molecular parameters of allergic lung inflammation were evaluated 24 h after the last Bt challenge. Exposure to eLPS but not to ultrapure LPS (upLPS) preparation during sensitization to Bt allergens decreased the influx of eosinophils and increased the influx of neutrophils to the airways. Inhibition of airway eosinophilia was not observed in IFN-γdeficient mice while airway neutrophilia was not observed in IL-17RA-deficient mice as well in mice lacking MyD88, CD14, TLR4 and, surprisingly, TLR2 molecules. Notably, exposure to a synthetic TLR2 agonist (PamCSK4) also induced airway neutrophilia that was dependent on TLR2 and TLR4 molecules. In the OVA model, exposure to eLPS or PamCSK4 suppressed OVA-induced airway inflammation. Our results suggest that B. tropicalis allergens engage TLR4 that potentiates TLR2 signaling. This dual TLR activation during sensitization results in airway neutrophilic inflammation associated with increased frequency of lung TH17 cells. Our work highlight the complex interplay between bacterial products, house dust mite allergens and TLR signaling in the induction of different phenotypes of airway inflammation.

Do the size shifts of marine macroalgae match the warming trends in the Canary Islands?

Departamento de Biología Vegetal (Botánica), Universidad de La Laguna, La Laguna, Canary Islands

Viruses in the marine environment: community dynamics, phage-host interactions and genomic structure

[EN] There are an estimated 1030 viruses in the world oceans, the majority of which are phages (viruses that infect bacteria). Extensive research has demonstrated the significant influence of marine phages on microbial abundance, community structure, genetic exchange and global biogeochemical cycles. In this thesis, we contribute to increase the knowledge about the ecological role of viruses in marine systems, but also we aimed to provide a better understanding about the interactions between phages and their hosts and the genetic pool and biogeography of some the isolated phages genomes.

Petroleum development and climate change: Risks of being a host country

Grabación realizada por Ciencia compartida (Biblioteca Universitaria)

Petroleum development and climate change: Risks of being a host country

[EN]A petroleum expert’s view on risks and benefits of oil exploration today in Canarias, considering the climate change facts. The talk starts with an overview of the total petroleum development process, from exploration to post-abandonment, indicating some important risks and benefits for each, from a petroleum industry and a personal perspective. Then there is a part of the talk about the agreed facts of climate change, and what this means for us all. The end of the talk brings together these two sections in a summary.

The VIMOS-VLT Deep Survey: the evolution of type-1 AGN

Quasars and AGN play an important role in many aspects of the modern cosmology. Of particular interest is the issue of the interplay between AGN activity and formation and evolution of galaxies and structures. Studies on nearby galaxies revealed that most (and possibly all) galaxy nuclei contain a super-massive black hole (SMBH) and that between a third and half of them are showing some evidence of activity (Kormendy and Richstone, 1995). The discovery of a tight relation between black holes mass and velocity dispersion of their host galaxy suggests that the evolution of the growth of SMBH and their host galaxy are linked together. In this context, studying the evolution of AGN, through the luminosity function (LF), is fundamental to constrain the theories of galaxy and SMBH formation and evolution. Recently, many theories have been developed to describe physical processes possibly responsible of a common formation scenario for galaxies and their central black hole (Volonteri et al., 2003; Springel et al., 2005a; Vittorini et al., 2005; Hopkins et al., 2006a) and an increasing number of observations in different bands are focused on collecting larger and larger quasar samples. Many issues remain however not yet fully understood. In the context of the VVDS (VIMOS-VLT Deep Survey), we collected and studied an unbiased sample of spectroscopically selected faint type-1 AGN with a unique and straightforward selection function. Indeed, the VVDS is a large, purely magnitude limited spectroscopic survey of faint objects, free of any morphological and/or color preselection. We studied the statistical properties of this sample and its evolution up to redshift z 4. Because of the contamination of the AGN light by their host galaxies at the faint magnitudes explored by our sample, we observed that a significant fraction of AGN in our sample would be missed by the UV excess and morphological criteria usually adopted for the pre-selection of optical QSO candidates. If not properly taken into account, this failure in selecting particular sub-classes of AGN could, in principle, affect some of the conclusions drawn from samples of AGN based on these selection criteria. The absence of any pre-selection in the VVDS leads us to have a very complete sample of AGN, including also objects with unusual colors and continuum shape. The VVDS AGN sample shows in fact redder colors than those expected by comparing it, for example, with the color track derived from the SDSS composite spectrum. In particular, the faintest objects have on average redder colors than the brightest ones. This can be attributed to both a large fraction of dust-reddened objects and a significant contamination from the host galaxy. We have tested these possibilities by examining the global spectral energy distribution of each object using, in addition to the U, B, V, R and I-band magnitudes, also the UV-Galex and the IR-Spitzer bands, and fitting it with a combination of AGN and galaxy emission, allowing also for the possibility of extinction of the AGN flux. We found that for 44% of our objects the contamination from the host galaxy is not negligible and this fraction decreases to 21% if we restrict the analysis to a bright subsample (M1450 <-22.15). Our estimated integral surface density at IAB < 24.0 is 500 AGN per square degree, which represents the highest surface density of a spectroscopically confirmed sample of optically selected AGN. We derived the luminosity function in B-band for 1.0 < z < 3.6 using the 1/Vmax estimator. Our data, more than one magnitude fainter than previous optical surveys, allow us to constrain the faint part of the luminosity function up to high redshift. A comparison of our data with the 2dF sample at low redshift (1 < z < 2.1) shows that the VDDS data can not be well fitted with the pure luminosity evolution (PLE) models derived by previous optically selected samples. Qualitatively, this appears to be due to the fact that our data suggest the presence of an excess of faint objects at low redshift (1.0 < z < 1.5) with respect to these models. By combining our faint VVDS sample with the large sample of bright AGN extracted from the SDSS DR3 (Richards et al., 2006b) and testing a number of different evolutionary models, we find that the model which better represents the combined luminosity functions, over a wide range of redshift and luminosity, is a luminosity dependent density evolution (LDDE) model, similar to those derived from the major Xsurveys. Such a parameterization allows the redshift of the AGN density peak to change as a function of luminosity, thus fitting the excess of faint AGN that we find at 1.0 < z < 1.5. On the basis of this model we find, for the first time from the analysis of optically selected samples, that the peak of the AGN space density shifts significantly towards lower redshift going to lower luminosity objects. The position of this peak moves from z 2.0 for MB <-26.0 to z 0.65 for -22< MB <-20. This result, already found in a number of X-ray selected samples of AGN, is consistent with a scenario of “AGN cosmic downsizing”, in which the density of more luminous AGN, possibly associated to more massive black holes, peaks earlier in the history of the Universe (i.e. at higher redshift), than that of low luminosity ones, which reaches its maximum later (i.e. at lower redshift). This behavior has since long been claimed to be present in elliptical galaxies and it is not easy to reproduce it in the hierarchical cosmogonic scenario, where more massive Dark Matter Halos (DMH) form on average later by merging of less massive halos.

A high energy perspective of the co-evolution of black holes and their host galaxies

Thanks to the Chandra and XMM–Newton surveys, the hard X-ray sky is now probed down to a flux limit where the bulk of the X-ray background is almost completely resolved into discrete sources, at least in the 2–8 keV band. Extensive programs of multiwavelength follow-up observations showed that the large majority of hard X–ray selected sources are identified with Active Galactic Nuclei (AGN) spanning a broad range of redshifts, luminosities and optical properties. A sizable fraction of relatively luminous X-ray sources hosting an active, presumably obscured, nucleus would not have been easily recognized as such on the basis of optical observations because characterized by “peculiar” optical properties. In my PhD thesis, I will focus the attention on the nature of two classes of hard X-ray selected “elusive” sources: those characterized by high X-ray-to-optical flux ratios and red optical-to-near-infrared colors, a fraction of which associated with Type 2 quasars, and the X-ray bright optically normal galaxies, also known as XBONGs. In order to characterize the properties of these classes of elusive AGN, the datasets of several deep and large-area surveys have been fully exploited. The first class of “elusive” sources is characterized by X-ray-to-optical flux ratios (X/O) significantly higher than what is generally observed from unobscured quasars and Seyfert galaxies. The properties of well defined samples of high X/O sources detected at bright X–ray fluxes suggest that X/O selection is highly efficient in sampling high–redshift obscured quasars. At the limits of deep Chandra surveys (∼10−16 erg cm−2 s−1), high X/O sources are generally characterized by extremely faint optical magnitudes, hence their spectroscopic identification is hardly feasible even with the largest telescopes. In this framework, a detailed investigation of their X-ray properties may provide useful information on the nature of this important component of the X-ray source population. The X-ray data of the deepest X-ray observations ever performed, the Chandra deep fields, allows us to characterize the average X-ray properties of the high X/O population. The results of spectral analysis clearly indicate that the high X/O sources represent the most obscured component of the X–ray background. Their spectra are harder (G ∼ 1) than any other class of sources in the deep fields and also of the XRB spectrum (G ≈ 1.4). In order to better understand the AGN physics and evolution, a much better knowledge of the redshift, luminosity and spectral energy distributions (SEDs) of elusive AGN is of paramount importance. The recent COSMOS survey provides the necessary multiwavelength database to characterize the SEDs of a statistically robust sample of obscured sources. The combination of high X/O and red-colors offers a powerful tool to select obscured luminous objects at high redshift. A large sample of X-ray emitting extremely red objects (R−K >5) has been collected and their optical-infrared properties have been studied. In particular, using an appropriate SED fitting procedure, the nuclear and the host galaxy components have been deconvolved over a large range of wavelengths and ptical nuclear extinctions, black hole masses and Eddington ratios have been estimated. It is important to remark that the combination of hard X-ray selection and extreme red colors is highly efficient in picking up highly obscured, luminous sources at high redshift. Although the XBONGs do not present a new source population, the interest on the nature of these sources has gained a renewed attention after the discovery of several examples from recent Chandra and XMM–Newton surveys. Even though several possibilities were proposed in recent literature to explain why a relatively luminous (LX = 1042 − 1043erg s−1) hard X-ray source does not leave any significant signature of its presence in terms of optical emission lines, the very nature of XBONGs is still subject of debate. Good-quality photometric near-infrared data (ISAAC/VLT) of 4 low-redshift XBONGs from the HELLAS2XMMsurvey have been used to search for the presence of the putative nucleus, applying the surface-brightness decomposition technique. In two out of the four sources, the presence of a nuclear weak component hosted by a bright galaxy has been revealed. The results indicate that moderate amounts of gas and dust, covering a large solid angle (possibly 4p) at the nuclear source, may explain the lack of optical emission lines. A weak nucleus not able to produce suffcient UV photons may provide an alternative or additional explanation. On the basis of an admittedly small sample, we conclude that XBONGs constitute a mixed bag rather than a new source population. When the presence of a nucleus is revealed, it turns out to be mildly absorbed and hosted by a bright galaxy.

Habitat shifts: an experimental study on disappearing canopies of Cystoseira barbata (Stackhouse) C. Agard and the habitat replacing them

Cambiamenti di habitat in ambienti marini: uno studio sperimentale sulla perdita di foreste a Cystoseira barbata (Stackhouse) C. Agardh e sui popolamenti che le sostituiscono La presente tesi affronta il tema scientifico generale di come prevedere e mitigare la perdita di habitat marini naturali causata dalle attività umane. La tesi si è focalizzata sugli habitat subtidali a “canopy” formati da macroalghe brune a tallo eretto dell’ordine Fucales, che per morfologia, ruolo ed importanza ecologica possono essere paragonate alle “foreste” in ambienti terrestri temperati. Questi sistemi sono tra i più produttivi in ambienti marini, e sono coinvolti in importanti processi ecologici, offrendo cibo, protezione, riparo ed ancoraggio a diverse altre specie animali e vegetali, modificando i gradienti naturali di luce, sedimentazione e idrodinamismo, e partecipando al ciclo dei nutrienti. Sulle coste temperate di tutto il mondo, le foreste di macroalghe a canopy sono in forte regressione su scala locale, regionale e globale. Questo fenomeno, che sta accelerando a un ritmo sempre più allarmante, sta sollevando interesse e preoccupazione. Infatti, data la loro importanza, la perdita di questi habitat può avere importanti conseguenze ecologiche ed economiche, tra cui anche il possibile declino della pesca che è stato osservato in alcune aree in seguito alla conseguente riduzione della produttività complessiva dei sistemi marini costieri. Nel Mar Mediterraneo questi tipi di habitat sono originati prevalentemente da alghe appartenenti al genere Cystoseira, che sono segnalate in forte regressione in molte regioni. Gli habitat a Cystoseira che ancora persistono continuano ad essere minacciati da una sineregia di impatti antropici, ed i benefici complessivi delle misure di protezione fin ora attuate sono relativamente scarsi. Scopo della presente tesi era quello di documentare la perdita di habitat a Cystoseira (prevalentemente Cystoseira barbata (Stackhouse) C. Agardh) lungo le coste del Monte Conero (Mar Adriatico centrale, Italia), e chiarire alcuni dei possibili meccanismi alla base di tale perdita. Studi precedentemente condotti nell’area di studio avevano evidenziato importanti cambiamenti nella composizione floristica e della distribuzione di habitat a Cystoseira in quest’area, e avevano suggerito che la scarsa capacità di recupero di questi sistemi potesse essere regolata da interazioni tra Cystoseira e le nuove specie dominanti sui substrati lasciati liberi dalla perdita di Cystoseira. Attraverso ripetute mappature dell’habitat condotte a partire da Luglio 2008 fino a Giugno 2010, ho documentato la perdita progressiva delle poche, e sempre più frammentate, patch di habitat originate da questa specie in due siti chiamati La Vela e Due Sorelle. Attraverso successivi esperimenti, ho poi evidenziato le interazioni ecologiche tra le specie dominanti coinvolte in questi cambiamenti di habitat, al fine di identificare possibili meccanismi di feedback che possano facilitare la persistenza di ciascun habitat o, viceversa, l’insediamento di habitat alternativi. La mappatura dell’habitat ha mostrato un chiaro declino della copertura, della densità e della dimensione degli habitat a Cystoseira (rappresentati soprattutto dalla specie C. barbata e occasionalmente C. compressa che però non è stata inclusa nei successivi esperimenti, d’ora in avanti per semplicità verrà utilizzato unicamente il termine Cystoseira per indicare questo habitat) durante il periodo di studio. Nel sito Due Sorelle le canopy a Cystoseira sono virtualmente scomparse, mentre a La Vela sono rimaste poche, sporadiche ed isolate chiazze di Cystoseira. Questi habitat a canopy sono stati sostituiti da nuovi habitat più semplici, tra cui soprattutto letti di mitili, feltri algali e stand monospecifici di Gracilaira spp.. La mappatura dell’habitat ha inoltre sottolineato una diminuzione del potenziale di recupero del sistema con un chiaro declino del reclutamento di Cystoseira durante tutto il periodo di studio. Successivamente ho testato se: 1) una volta perse, il recupero di Cystoseira (reclutamento) possa essere influenzato dalle interazioni con le nuove specie dominanti, quali mitili e feltri algali; 2) il reclutamento di mitili direttamente sulle fronde di Cystoseira (sia talli allo stadio adulto che giovanili) possa influenzare la sopravvivenza e la crescita della macroalga; 3) la sopravvivenza e la crescita delle nuove specie dominanti, in particolare mitili, possa essere rallentata dalla presenza di canopy di Cystoseira. I risultati dimostrano che le nuove specie dominanti insediatesi (feltri algali e mitili), possono inibire il reclutamento di Cystoseira, accelerandone il conseguente declino. L’effetto diretto dei mitili sulle fronde non è risultato particolarmente significativo né per la sopravvivenza di Cystoseira che finora non è risultata preclusa in nessun stadio di sviluppo, né per la crescita, che nel caso di individui adulti è risultata leggermente, ma non significativamente, più elevata per le fronde pulite dai mitili, mentre è stato osservato il contrario per i giovanili. La presenza di canopy a Cystoseira, anche se di piccole dimensioni, ha limitato la sopravvivenza di mitili. Questi risultati complessivamente suggeriscono che una foresta di macroalghe in buone condizioni può avere un meccanismo di autoregolazione in grado di facilitare la propria persistenza. Quando però il sistema inizia a degradarsi e a frammentarsi progressivamente, i cambiamenti delle condizioni biotiche determinati dall’aumento di nuove specie dominanti contribuiscono alla mancanza di capacità di recupero del sistema. Pertanto le strategie per una gestione sostenibile di questi sistemi dovrebbero focalizzarsi sui primi segnali di cambiamenti in questo habitat e sui possibili fattori che ne mantengono la resilienza.

Ground state properties of neutron-rich Mg isotopes

Studies in regions of the nuclear chart in which the model predictions of properties of nuclei fail can bring a better understanding of the strong interaction in the nuclear medium. To such regions belongs the so called "island of inversion" centered around Ne, Na and Mg isotopes with 20 neutrons in which unexpected ground-state spins, large deformations and dense low-energy spectra appear. This is a strong argument that the magic N = 20 is not a closed shell in this area. In this thesis investigations of isotope shifts of stable 24,25,26Mg, as well as spins and magnetic moments of short-lived 29,31Mg are presented. The successful studies were performed at the ISOLDE facility at CERN using collinear laser and beta-NMR spectroscopy techniques. The isotopes were investigated as single-charged ions in the 280-nm transition from the atomic ground state 2S1/2 to one of the two lowest excited states 2P1/2,3/2 using continuous wave laser beams. The isotope-shift measurements with fluorescence detection for the three stable isotopes show that it is feasible to perform the same studies on radioactive Mg isotopes up to the "island of inversion". This will allow to determine differences in the mean charge square radii and interpret them in terms of deformation. The high detection efficiency for beta particles and optical pumping close to saturation allowed to obtain very good beta-asymmetry signals for 29Mg and 31Mg with half-lives around 1 s and production yields about 10^5 ions/s. For this purpose the ions were implanted into a host crystal lattice. Such detection of the atomic resonances revealed their hyperfine structure, which gives the sign and a first estimate of the value of the magnetic moment. The nuclear magnetic resonance gave also their g-factors with the relative uncertainty smaller than 0.2 %. By combining the two techniques also the nuclear spin of both isotopes could be unambiguously determined. The measured spins and g-factors show that 29Mg with 17 neutrons lies outside the "island of inversion". On the other hand, 31Mg with 19 neutrons has an unexpected ground-state spin which can be explained only by promoting at least two neutrons across the N = 20 shell gap. This places the above nucleus inside the "island". However, modern shell-model approaches cannot predict this level as the ground state but only as one of the low-lying states, even though they reproduce very well the experimental g-factor. This indicates that modifications to the available interactions are required. Future measurements include isotope shift measurements on radioactive Mg isotopes and beta-NMR studies on 33Mg.

Bifidobacterium - Human Host Interaction: Role of Human Plasminogen

Bifidobacterium is an important genus of the human gastrointestinal microbiota, affecting several host physiological features. Despite the numerous Bifidobacterium related health-promoting activities, there is still a dearth of information about the molecular mechanisms at the basis of the interaction between this microorganism and the host. Bacterial surface associated proteins may play an important role in this interaction because of their ability to intervene with host molecules, as recently reported for the host protein plasminogen. Plasminogen is the zymogen of the trypsin-like serine protease plasmin, an enzyme with a broad substrate specificity. Aim of this thesis is to deepen the knowledge about the interaction between Bifidobacterium and the human plasminogen system and its role in the Bifidobacterium-host interaction process. As a bifidobacterial model, B. animalis subsp. lactis BI07 has been used because of its large usage in dairy and pharmaceutical preparations. We started from the molecular characterization of the interaction between plasminogen and one bifidobacterial plasminogen receptor, DnaK, a cell wall protein showing high affinity for plasminogen, and went on with the study of the impact of intestinal environmental factors, such as bile salts and inflammation, on the plasminogen-mediated Bifidobacterium-host interaction. According to our in vitro findings, by enhancing the activation of the bifidobacterial bound plasminogen to plasmin, the host inflammatory response results in the decrease of the bifidobacterial adhesion to the host enterocytes, favouring bacterial migration to the luminal compartment. Conversely, in the absence of inflammation, plasminogen acts as a molecular bridge between host enterocytes and bifidobacteria, enhancing Bifidobacterium adhesion. Furthermore, adaptation to physiological concentrations of bile salts enhances the capability of this microorganism to interact with the host plasminogen system. The host plasminogen system thus represents an important and flexible tool used by bifidobacteria in the cross-talk with the host.

The influence of heat treatment on the phase relations in mineral growth systems

ABSTRACT Corundum is one of the most famous gems materials. Different heat treatment methods for enhancement purposes are commonly applied and accepted in the gem market. With this reason, the identification of the natural, unheated corundum is intensively investigated. In this study, aluminium hydroxide minerals and zircon are focused to observe the crystallization and phase change of these minerals during heat treatment procedures. Aluminium hydroxide minerals can be transformed to alumina with the corundum structure by heating. The reaction history of aluminium hydroxide minerals containing corundum was investigated comparing it with diaspore, boehmite, gibbsite and bayerite by TG and DTA methods. These hydroxide minerals were entirely transformed to corundum after heating at 600°C. Zircon inclusions in corundums from Ilakaka, Madagascar, were investigated for the influence of different heat-treatment temperatures on the recovery of their crystalline structure and on possible reactions within and with the host crystals. The host corundum was heated at 500, 800, 1000, 1200, 1400, 1600 and 1800°C. The crystallinity, the trapped pressure, and the decomposition of the zircon inclusions within the host corundum have been investigated by Raman spectroscopy. Radiation-damaged zircon inclusions may be used as an indicator for unheated Ilakaka corundum crystals. They are fully recrystallized after heating at 1000°C influencing the lowering of the 3 Raman band shift, the decreasing of FWHM of the 3 Raman band and the decreasing of the trapped pressure between the inclusion and the host corundum. Under microscopic observation, surface alterations of the inclusions can be firstly seen from transparent into frosted-like appearance at 1400°C. Then, between 1600°C and 1800 °C, the inclusion becomes partly or even completely molten. The decomposition of the zircon inclusion to m-ZrO2 and SiO2-glass phases begins at the rim of the inclusion after heating from 1200°C to 1600°C which can be detected by the surface change, the increase of the 3 Raman band position and the trapped pressure. At 1800°C, the zircon inclusions entirely melt transforming to solid phases during cooling like m-ZrO2 and SiO2-glass accompanied by an increase of pressure between the transformed inclusion and its host.

13C NMR of a single molecule magnet: analysis of pseudocontact shifts and residual dipolar couplings

Paramagnetic triple decker complexes of lanthanides are promising Single Molecule Magnets (SMMs), with many potential uses. Some of them show preferable relaxation behavior, which enables the recording of well resolved NMR spectra. These axially symmetric complexes are also strongly magnetically anisotropic, and this property can be described with the axial component of the magnetic susceptibility tensor, χa. For triple decker complexes with phthalocyanine based ligands, the Fermi˗contact contribution is small. Hence, together with the axial symmetry, the experimental chemical shifts in 1H and 13C NMR spectra can be modeled easily by considering pseudocontact and orbital shifts alone. This results in the determination of the χa value, which is also responsible for molecular alignment and consequently for the observation of residual dipolar couplings (RDCs). A detailed analysis of the experimental 1H-13C and 1H-1H couplings revealed that contributions from RDCs (positive and negative) and from dynamic frequency shifts (negative for all observed couplings) have to be considered. Whilst the pseudocontact shifts depend on the average positions of 1H and 13C nuclei relative to the lanthanide ions, the RDCs are related to the mobility of nuclei they correspond to. This phenomenon allows for the measurement of the internal mobility of the various groups in the SMMs.

Host immune response in immunodeficient mice against infection with Cryptosporidium parvum

Immunantwort von immundefizienten Mäusen gegenüber Infektionen mit Cryptosporidium parvum. Cryptosporidium parvum ist ein intrazellulärer, protozoischer Krankheitserreger, der im immunkompromittierten Wirt zu lebensbedrohender Enteritis führen kann. CD4+ T-Zellen und Interferon (IFN)-γ spielen wesentliche Rollen bei der Wirtsimmunantwort gegen die Infektion. Dennoch sind die Effektormechanismen, die zur Resistenz führen nur wenig verstanden. In dieser Studie wurde die Immunantwort von IFN-γ- und Interleukin (IL)-12-Defektmäusen parallel zu Wildtypmäusen analysiert. Die Ergebnisse identifizierten IFN-γ als Schlüsselzytokin bei der natürlichen und erworbenen Immunität während der Erst- und Folgeinfektion mit C. parvum. Tumornekrosefaktor (TNF)-α ist möglicherweise ein Induktor der frühen IFN-γ-Antwort in IL-12 Knockout-Mäusen. Weiterhin tragen offenbar sowohl Th1- als auch Th2-Zytokine zur Überwindung der Primärinfektion bei, die ersten mehr als die letztgenannten. Zytokingene waren am Ort der Infektion (Ileum) dramatisch verändert, nicht aber in den lokalen Lymphknoten und der Milz. Nach Folgeinfektion ergab sich in Abwesenheit von IFN-γ eine signifikante Erhöhung der Th2-Zytokine IL-5 and IL-13. Die Ergebnisse zeigten weiterhin, dass das Th1-Zytokin IL-18 zur Resistenz gegenüber C. parvum beiträgt, möglicherweise durch verschiedene Immunfunktionen, wie der Regulation von Serum-IFN-γ während der Infektion und/oder der Erhaltung der Homeostase der Th1/Th2-Zytokine durch Regulation der Th2-Zytokine. Weiterhin zeigten diese Untersuchungen den Transfer von Resistenz gegenüber C. parvum von infizierten auf naïve Mäuse mittels stimulierter intraepithelialer Lymphozyten und CD4+ T-Zellen. Diese Ergebnisse weisen auf die Gegenwart von C. parvum-spezifischen CD4+ T-Zellen in anderen lymphatischen Geweben neben der Darmmukosa hin. Eine Stimulation der Spendertiere durch Infektion war notwendig für eine übertragbare schützende Immunität. Dennoch konnte die übertragene Immunität nicht die Infektion der Empfängertiere vollständig verhindern; eine Verdopplung der Spenderzellen führte zu keinem besseren Ergebnis. Weiterhin ergab der Transfer von CD4+ und CD8+ T-Zellen (Pan-T-Zellen) keinen erhöhten Schutz der naiven Empfängertiere als der alleinige Transfer von CD4+ T-Zellen. Dies weist auf die fehlende Bedeutung der CD8+ T-Zellen beim Schutz vor C. parvum-Infektion hin.