984 resultados para Vannozzi, Bonifazio, 1551-1627.


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Programa de doctorado: Literatura y Teoría de la Literatura

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Seyfert galaxies are the closest active galactic nuclei. As such, we can use them to test the physical properties of the entire class of objects. To investigate their general properties, I took advantage of different methods of data analysis. In particular I used three different samples of objects, that, despite frequent overlaps, have been chosen to best tackle different topics: the heterogeneous BeppoS AX sample was thought to be optimized to test the average hard X-ray (E above 10 keV) properties of nearby Seyfert galaxies; the X-CfA was thought the be optimized to compare the properties of low-luminosity sources to the ones of higher luminosity and, thus, it was also used to test the emission mechanism models; finally, the XMM–Newton sample was extracted from the X-CfA sample so as to ensure a truly unbiased and well defined sample of objects to define the average properties of Seyfert galaxies. Taking advantage of the broad-band coverage of the BeppoS AX MECS and PDS instruments (between ~2-100 keV), I infer the average X-ray spectral propertiesof nearby Seyfert galaxies and in particular the photon index (~1.8), the high-energy cut-off (~290 keV), and the relative amount of cold reflection (~1.0). Moreover the unified scheme for active galactic nuclei was positively tested. The distribution of isotropic indicators used here (photon index, relative amount of reflection, high-energy cut-off and narrow FeK energy centroid) are similar in type I and type II objects while the absorbing column and the iron line equivalent width significantly differ between the two classes of sources with type II objects displaying larger absorbing columns. Taking advantage of the XMM–Newton and X–CfA samples I also deduced from measurements that 30 to 50% of type II Seyfert galaxies are Compton thick. Confirming previous results, the narrow FeK line is consistent, in Seyfert 2 galaxies, with being produced in the same matter responsible for the observed obscuration. These results support the basic picture of the unified model. Moreover, the presence of a X-ray Baldwin effect in type I sources has been measured using for the first time the 20-100 keV luminosity (EW proportional to L(20-100)^(−0.22±0.05)). This finding suggests that the torus covering factor may be a function of source luminosity, thereby suggesting a refinement of the baseline version of the unifed model itself. Using the BeppoSAX sample, it has been also recorded a possible correlation between the photon index and the amount of cold reflection in both type I and II sources. At a first glance this confirms the thermal Comptonization as the most likely origin of the high energy emission for the active galactic nuclei. This relation, in fact, naturally emerges supposing that the accretion disk penetrates, depending to the accretion rate, the central corona at different depths (Merloni et al. 2006): the higher accreting systems hosting disks down to the last stable orbit while the lower accreting systems hosting truncated disks. On the contrary, the study of the well defined X–C f A sample of Seyfert galaxies has proved that the intrinsic X-ray luminosity of nearby Seyfert galaxies can span values between 10^(38−43) erg s^−1, i.e. covering a huge range of accretion rates. The less efficient systems have been supposed to host ADAF systems without accretion disk. However, the study of the X–CfA sample has also proved the existence of correlations between optical emission lines and X-ray luminosity in the entire range of L_(X) covered by the sample. These relations are similar to the ones obtained if high-L objects are considered. Thus the emission mechanism must be similar in luminous and weak systems. A possible scenario to reconcile these somehow opposite indications is assuming that the ADAF and the two phase mechanism co-exist with different relative importance moving from low-to-high accretion systems (as suggested by the Gamma vs. R relation). The present data require that no abrupt transition between the two regimes is present. As mentioned above, the possible presence of an accretion disk has been tested using samples of nearby Seyfert galaxies. Here, to deeply investigate the flow patterns close to super-massive black-holes, three case study objects for which enough counts statistics is available have been analysed using deep X-ray observations taken with XMM–Newton. The obtained results have shown that the accretion flow can significantly differ between the objects when it is analyzed with the appropriate detail. For instance the accretion disk is well established down to the last stable orbit in a Kerr system for IRAS 13197-1627 where strong light bending effect have been measured. The accretion disk seems to be formed spiraling in the inner ~10-30 gravitational radii in NGC 3783 where time dependent and recursive modulation have been measured both in the continuum emission and in the broad emission line component. Finally, the accretion disk seems to be only weakly detectable in rk 509, with its weak broad emission line component. Finally, blueshifted resonant absorption lines have been detected in all three objects. This seems to demonstrate that, around super-massive black-holes, there is matter which is not confined in the accretion disk and moves along the line of sight with velocities as large as v~0.01-0.4c (whre c is the speed of light). Wether this matter forms winds or blobs is still matter of debate together with the assessment of the real statistical significance of the measured absorption lines. Nonetheless, if confirmed, these phenomena are of outstanding interest because they offer new potential probes for the dynamics of the innermost regions of accretion flows, to tackle the formation of ejecta/jets and to place constraints on the rate of kinetic energy injected by AGNs into the ISM and IGM. Future high energy missions (such as the planned Simbol-X and IXO) will likely allow an exciting step forward in our understanding of the flow dynamics around black holes and the formation of the highest velocity outflows.

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Precision horticulture and spatial analysis applied to orchards are a growing and evolving part of precision agriculture technology. The aim of this discipline is to reduce production costs by monitoring and analysing orchard-derived information to improve crop performance in an environmentally sound manner. Georeferencing and geostatistical analysis coupled to point-specific data mining allow to devise and implement management decisions tailored within the single orchard. Potential applications range from the opportunity to verify in real time along the season the effectiveness of cultural practices to achieve the production targets in terms of fruit size, number, yield and, in a near future, fruit quality traits. These data will impact not only the pre-harvest but their effect will extend to the post-harvest sector of the fruit chain. Chapter 1 provides an updated overview on precision horticulture , while in Chapter 2 a preliminary spatial statistic analysis of the variability in apple orchards is provided before and after manual thinning; an interpretation of this variability and how it can be managed to maximize orchard performance is offered. Then in Chapter 3 a stratification of spatial data into management classes to interpret and manage spatial variation on the orchard is undertaken. An inverse model approach is also applied to verify whether the crop production explains environmental variation. In Chapter 4 an integration of the techniques adopted before is presented. A new key for reading the information gathered within the field is offered. The overall goal of this Dissertation was to probe into the feasibility, the desirability and the effectiveness of a precision approach to fruit growing, following the lines of other areas of agriculture that already adopt this management tool. As existing applications of precision horticulture already had shown, crop specificity is an important factor to be accounted for. This work focused on apple because of its importance in the area where the work was carried out, and worldwide.

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La presente tesi descrive l’implementazione in Java di un algoritmo per il ragionamento giuridico che cattura due sue importanti peculiarità: la defeasibility del ragionamento normativo e il concetto di tempo. “Defeasible” significa “ritrattabile” e sta ad indicare, appunto, quegli schemi di ragionamento nei quali è possibile rivedere o ritrattare le conclusioni tratte precedentemente. Il tempo è essenziale per un’accurata rappresentazione degli scenari presenti nel mondo reale e in particolare per gli scenari giuridici. I profili temporali delle norme sono essenzialmente due: (i) tempo esterno della norma, cioè il periodo durante il quale la norma è valida cioè appartiene al sistema giuridico; (ii) tempo interno della norma che fa riferimento al periodo in cui la norma si applica. In particolare quest’ultimo periodo di tempo coincide con il periodo in cui le condizioni presenti nella norma devono presentarsi affinché essa produca i suoi effetti. Inoltre, nella tesi viene presentata un’estensione della logica defeasible in grado di distinguere tra regole con effetti persistenti, che valgono non solo per l’istante in cui si verificano le premesse ma anche per ogni istante successivo, e regole con effetti transitori, che valgono per un singolo istante. L’algoritmo presentato in questa tesi presenta una complessità lineare nelle dimensioni della teoria in ingresso e può interagire con le applicazioni del web semantico poiché elabora teorie scritte in Rule-ML, un linguaggio basato su XML per la rappresentazione di regole.

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Il lavoro ripercorre le tracce che gli ebrei portoghesi, esuli dopo il biennio 1496-97, lasciarono nel loro cammino attraverso l'Europa. In particolare, l'interesse si concentra sulla breve parentesi italiana, che grazie all'apertura e alla disponibilità  di alcuni Signori, come i Gonzaga di Mantova, i Medici, i Dogi della Serenissima e gli Este, risulta ricchissima di avvenimenti e personaggi, decisivi anche per la storia culturale del Portogallo. L'analisi parte evidenziando l'importanza che ebbe la tipografia ebraica in Portogallo all'epoca della sua introduzione nel Paese; in secondo luogo ripercorre la strada che, dal biennio del primo decreto di espulsione e del conseguente battesimo di massa, porta alla nascita dell'€™Inquisizione in Portogallo. Il secondo capitolo tenta di fare una ricostruzione, il più possibile completa e coerente, dei movimenti degli esuli, bollati come marrani e legati alle due maggiori famiglie, i Mendes e i Bemveniste, delineando poi il primo nucleo di quella che diventerà  nel Seicento la comunità  sefardita portoghese di Amsterdam, dove nasceranno le personalità  dissidenti di Uriel da Costa e del suo allievo Spinoza. Il terzo capitolo introduce il tema delle opere letterarie, effettuando una rassegna dei maggiori volumi editi dalle officine tipografiche ebraiche stanziatesi in Italia fra il 1551 e il 1558, in modo particolare concentrando l'attenzione sull'€™attività  della tipografia Usque, da cui usciranno numerosi testi di precettistica in lingua ebraica, ma soprattutto opere cruciali come la famosa «Bibbia Ferrarese» in castigliano, la «Consolação às Tribulações de Israel», di Samuel Usque e la raccolta composta dal romanzo cavalleresco «Menina e Moça» di Bernardim Ribeiro e dall'ecloga «Crisfal», di un autore ancora non accertato. L'ultimo capitolo, infine, si propone di operare una disamina di queste ultime tre opere, ritenute fondamentali per ricostruire il contesto letterario e culturale in cui la comunità  giudaica in esilio agiva e proiettava le proprie speranze di futuro. Per quanto le opere appartengano a generi diversi e mostrino diverso carattere, l'€™ipotesi è che siano parte di un unicum filosofico e spirituale, che intendeva sostanzialmente indicare ai confratelli sparsi per l'Europa la direzione da prendere, fornendo un sostegno teoretico, psicologico ed emotivo nelle difficili condizioni di sopravvivenza, soprattutto dell'integrità religiosa, di ciascun membro della comunità.

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Beim Beobachten von nächtlichen Insektenschwärmen an Straßenbeleuchtungen kommt es zur Frage, inwieweit von einer Bedrohung eines geordneten Naturkreislaufes durch dieses Phänomen gesprochen werden kann. Am Beispiel der bedrohten Artenvielfalt aquatischer Insekten im Bereich anthropogen bedingt verschmutzter Fließgewässer wurde die Problematik umfassend untersucht. Die Freilandtests erstreckten sich von Sommer 1998 bis Sommer 2000. Die vorliegende Arbeit geht mehreren Fragestellungen nach:1. - Wie hoch ist der Anteil aquatischer Insekten, der von dem Ort seiner Emergenz aus von einer naheliegenden Straßenlaterne angezogen wird ?2. - Welcher Lampentyp lockt weniger Insekten an: OSRAM HQL (Weiß-Mischlicht) oder PHILIPPS SON (gelbes Licht) ?3. - Welche Wellenlängenbereiche des Lichts sind beim Anflug an die Lampe von besonderer Präferenz ? zu 1. - Aquatische Insekten wiesen kein einheitliches Verhalten im Anflug an künstliches Licht auf. In den Sommermonaten kam es bei einigen Insektengruppen, wie z.B. den Trichopteren, zu einem massenhaften Anflug an die eine, im Untersuchungsgebiet aufgestellte Straßenlaterne. In dieser Zeit ergaben sich im Mittelwert Fangzahlen in einer Nacht am Licht, die der Emergenz von 25 Metern Bachufer/72 Stunden entsprachen. Bei den Dipteren ergab der mittlere Wert eine Emergenz von knapp 10 Metern Uferlänge/72 Stunden. Aufgrund hoher Fangzahlen konnten folgende Ergebnisse auf Artniveau bei den Chironomiden erzielt werden. Bei den zehn häufigsten Arten aus Emergenz und Lichtfang zeigten sich starke Schwankungen: Der Fang am Licht entsprach im Maximum einer Schlupfrate von 61 Metern Ufer/ 72 Stunden bei einer Art, bei einer anderen Art wurde z.B. ein Lichtfang erzielt, der lediglich die Emergenz von 0,3 Metern/72 Stunden umfaßte.zu 2. - In dem ohne Lichtkonkurrenz stattfindenden Vergleich zwischen PHILIPPS SON 70W und OSRAM HQL 125W ergab sich eine Fangrelation von 1:1,6 (SON:HQL). Bei einem Parallelfang (30 Metern Abstand der Leuchten) mit SON/HQL flogen wesentlich mehr Tiere an die HQL: Hier betrug die Relation 1:3,97 (SON:HQL). Es fand somit bei Lichtkonkurrenz eine Abwanderung der Insekten zur 'attraktiveren' Lampe statt.zu 3. - Zuletzt wurde die Anlockwirkung dreier Farbspektren mit den Intensitätsmaxima einer Wellenlänge von 437nm, 579nm und 599nm getestet. 437nm war die in der HQL gemessene Intensitätsspitze im niedrigwelligen Bereich und nach verbreiteter Auffassung von besonderer Anlockwirkung. Der Wellenlängenbereich um 579nm stellte das Intensitätsmaximum der SON-Lampe dar (gelbes Licht); 599nm war als Alternative für anlockschwache Beleuchtungen ausgewählt worden. Hier ergab sich bei abwechselndem Fang (ohne Lichtkonkurrenz) eine Fangrelation von 1,8 : 3,4 : 1 (437nm : 579nm : 599nm).

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Hämocyanine sind große, kupferhaltige Sauerstoff-Transportproteine, die bei zahlreichen Schnecken extrazellulär in der Hämolymphe vorkommen. Das Keyhole Limpet-Hämocyanin (KLH) der Schlüssellochschnecke Megathura crenulata dient aufgrund seiner immunstimu-latorischen Eigenschaften seit vielen Jahren als Modellprotein in der Immunologie. In der Klinik wird es als Hapten- und Vakzincarrier sowie als Medikament gegen oberflächliche Harnblasenkarnzinome eingesetzt. Die Quartärstruktur des KLH besteht aus einem Hohl-zylinder mit einer Molekülmasse von 8 MDa und einem Durchmesser von 35 nm. Dieses sogenannte Didekamer setzt sich aus 20 Untereinheiten mit jeweils 400 kDa zusammen. Jede Untereinheit lässt sich weiter in acht funktionelle Einheiten a bis h (engl. Functional Units = FU) mit ~ 50 kDa unterteilen. Die FUs a bis f bilden die Wandregion des Moleküls, während der Kragen aus den FUs g und h geformt wird. Die Struktur der Wandregion sowie der FU-g konnte bisher bereits durch Röntgenstrukturanalysen aufgeklärt werden. Bezüglich der Struktur der FU-h, die sich durch eine spezielle C-terminale Verlängerung von ~ 100 Amino-säuren auszeichnet, sind allerdings noch keine Informationen verfügbar. Um die Architektur des Kragens zu verstehen, wurden im Rahmen dieser Arbeit zunächst Strategien entwickelt, diese spezielle FU in großer Menge und Reinheit zu isolieren. Anschließend konnten Bedingungen gefunden werden, die zur Ausbildung 0,2 mm großer, hexagonaler Kristalle führten. Diese ergaben am Synchrotron eine Auflösung von 4 Å. Durch Auswertung der Röntgenstrukturdaten konnte für die C-terminale Zusatzdomäne der FU-h eine Cupredoxin-ähnliche Typ I-Kupferfaltung ermittelt werden. Der Nachweis eines zusätzlichen Kupfer-atoms innerhalb dieser Domäne bedarf allerdings einer höheren Auflösung der Kristall-struktur. Hämocyanine lassen sich aufgrund ihrer evolutionären Verwandtschaft zu Phenol-oxidasen mit Hilfe verschiedener in vitro-Aktivatoren zur Catecholoxidase und teilweise auch zur Tyrosinase aktivieren. Beim KLH konnte in dieser Arbeit eine eindeutige Diphenolase- und sogar eine schwache Monophenolase-Aktivität der FUs-a und -f nach SDS-Aktivierung nachgewiesen werden. Zudem konnte eine geringfügige intrinsische Diphenolase-Aktivität dieser FUs belegt werden. Die enzymatischen Reaktionen waren sowohl von der gewählten Puffersubstanz, als auch der Anwesenheit bivalenter Kationen abhängig. Tris wirkt vermutlich als allosterischer Effektor und steigerte den Substrat-Umsatz, während Mg2+-Ionen zu einer starken Inhibition der katalytischen Aktivität führten. Die Klärung einer möglichen physiologischen Funktion der Phenoloxidase-Aktivität des KLH sowie potenziellen in vivo-Aktivatoren steht noch aus. Studien zur thermischen Stabilität des KLH resultierten in einer irreversiblen Denaturierung des Proteins. Die Schmelzpunkte deuteten auf eine hohe Tempe-raturstabilität des KLH, vor allem in Anwesenheit bivalenter Kationen. Eine Hämocyanin-typische Abhängigkeit der Hitzeresistenz vom Oligomerisierungsgrad ließ sich nicht feststellen, da sowohl bei der FU-h als auch den KLH-Didekameren eine vergleichbar hohe thermische Stabilität, bei einer nach wie vor vorhandenen Oxygenierung beobachtet wurde.

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Peptide receptor targeting has become an increasingly attractive method to target tumors diagnostically and radiotherapeutically. Peptides linked to a variety of chelators have been developed for this purpose. They have, however, rarely been tested for their agonistic or antagonistic properties. We report here on a somatostatin antagonist that switched to an agonist upon coupling to a DOTA chelator.

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The aim of the study was to examine the clinical forensic findings of strangulation according to their ability to differentiate between life-threatening and non-life-threatening strangulation, compare clinical and MRI findings of the neck and discuss a simple score for life-threatening strangulation (SLS).

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The first generation of the bioresorbable everolimus drug-eluting vascular scaffold showed signs of shrinkage at 6 months, which largely contributed to late luminal loss. Nevertheless, late luminal loss was less than that observed with bare metal stents. To maintain the mechanical integrity of the device up to 6 months, the scaffold design and manufacturing process of its polymer were modified.

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Uncoated self-expanding nitinol stents (NS) are commonly oversized in peripheral arteries. In current practice, 1-mm oversizing is recommended. Yet, oversizing of NS may be associated with increased restenosis. To provide further evidence, NS were implanted in porcine iliofemoral arteries with a stent-to-artery-ratio between 1.0 and 2.3. Besides conventional uncoated NS, a novel self-expanding NS with an antiproliferative titanium-nitride-oxide (TiNOX) coating was tested for safety and efficacy.

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The cannabinoid system (CS) is implicated in the regulation of hepatic fibrosis, steatosis and inflammation, with cannabinoid receptors 1 and 2 (CB1 and CB2) being involved in regulation of pro- and antifibrogenic effects. Daily cannabis smoking is an independent risk factor for the progression of fibrosis in chronic hepatitis C and a mediator of experimental alcoholic steatosis. However, the role and function of CS in alcoholic liver fibrosis (ALF) is unknown so far. Thus, human liver samples from patients with alcoholic liver disease (ALD) were collected for analysis of CB1 expression. In vitro, hepatic stellate cells (HSC) underwent treatment with acetaldehyde, Δ9-tetrahydrocannabinol H(2)O(2), endo- and exocannabinoids (2-arachidonoylglycerol (2-AG) and [THC]), and CB1 antagonist SR141716 (rimonabant). In vivo, CB1 knockout (KO) mice received thioacetamide (TAA)/ethanol (EtOH) to induce fibrosis. As a result, in human ALD, CB1 expression was restricted to areas with advanced fibrosis only. In vitro, acetaldehyde, H(2)O(2), as well as 2-AG and THC, alone or in combination with acetaldehyde, induced CB1 mRNA expression, whereas CB1 blockage with SR141716 dose-dependently inhibited HSC proliferation and downregulated mRNA expression of fibrosis-mediated genes PCα1(I), TIMP-1 and MMP-13. This was paralleled by marked cytotoxicity of SR141716 at high doses (5-10 μmol/L). In vivo, CB1 knockout mice showed marked resistance to alcoholic liver fibrosis. In conclusion, CB1 expression is upregulated in human ALF, which is at least in part triggered by acetaldehyde (AA) and oxidative stress. Inhibition of CB1 by SR141716, or via genetic knock-out protects against alcoholic-induced fibrosis in vitro and in vivo.