903 resultados para Blue shift
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Miquel Becerro es científico del Instituto de Productos Naturales y Agrobiología -IPNA- (CSIC)
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L’idrogeno è un elemento di elevato interesse economico, con una produzione industriale che supera i 55 x 1010 m3/anno e notevoli prospettive di sviluppo delle sue applicazioni. Attualmente l’idrogeno è prodotto principalmente in impianti di larga scala (circa 1000 m3/h) da combustibili fossili attraverso processi di steam reforming ed ossidazione parziale catalitica. Per aumentare la produzione di idrogeno un ruolo fondamentale è svolto dalla reazione di water gas shift (WGS) che abbatte il contenuto di CO, massimizzando la produzione di idrogeno. La reazione è condotta industrialmente in due stadi, operanti ad alta temperatura (HTS, circa 350 °C) e bassa temperatura (LTS, circa 250 °C), utilizzando rispettivamente catalizzatori a base di ferro o rame. Tuttavia, è evidente l’interesse per nuove formulazioni in grado di operare in un unico stadio a temperatura intermedia (MTS), mantenendo le caratteristiche ottimali di attività e stabilità. In questo lavoro di tesi, condotto in collaborazione con AIR LIQUIDE (F), è stato affrontato uno studio della reazione di WGS finalizzato allo sviluppo di nuove formulazioni attive e stabili nell’MTS. In particolare, sono stati sintetizzati precursori idrotalcitici Cu/Zn/Al (contenenti carbonati o silicati), con bassi contenuti di rame (diversamente da quanto riportato in letteratura), modulandone le proprietà chimico-fisiche, l’attività catalitica e la stabilità con il tempo di reazione. Si è osservato come i catalizzatori con minori contenuti di rame ed ottenuti da precursori contenenti carbonati mostrassero un’elevata attività e selettività nell’MTS, raggiungendo valori di conversione del CO analoghi a quelli all’equilibrio termodinamico già a 300 °C, indipendentemente dai valori del rapporto S/DG e del tempo di contatto. Tutti i catalizzatori mostrano un’elevata stabilità con il tempo di reazione, con incrementi del quantitativo del CO in uscita dopo 100h di circa lo 0,7 % v/v. I catalizzatori scaricati dopo le prove catalitiche evidenziano gli effetti dei processi di sinterizzazione (diminuzione dell’area superficiale ed incremento delle dimensioni dei cristalliti), la cui entità diminuisce al diminuire del contenuto di rame. Infine, confrontando l’attività dei migliori catalizzatori preparati in questo lavoro di tesi con quella di uno dei più utilizzati catalizzatori commerciali per la reazione di WGS a bassa temperatura, si sono osservati valori di attività analoghi, raggiungendo quelli di equilibrio per temperature 300°C, ma con una attività significativamente superiore nelle condizioni LTS, soprattutto considerando il valore del tempo di contatto inferiore a quelli comunemente utilizzati negli impianti industriali.
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H2 demand is continuously increasing since its many relevant applications, for example, in the ammonia production, refinery processes or fuel cells. The Water Gas Shift (WGS) reaction (CO + H2O = CO2 + H2 DeltaH = -41.1 kJ.mol-1) is a step in the H2 production, reducing significantly the CO content and increasing the H2 one in the gas mixtures obtained from steam reforming. Industrially, the reaction is carried out in two stages with different temperature: the first stage operates at high temperature (350-450 °C) using Fe-based catalysts, while the second one is performed at lower temperature (190-250 °C) over Cu-based catalysts. However, recently, an increasing interest emerges to develop new catalytic formulations, operating in a single-stage at middle temperature (MTS), while maintaining optimum characteristics of activity and stability. These formulations may be obtained by improving activity and selectivity of Fe-based catalysts or increasing thermal stability of Cu-based catalysts. In the present work, Cu-based catalysts (Cu/ZnO/Al2O3) prepared starting from hydrotalcite-type precursors show good homogeneity and very interesting physical properties, which worsen by increasing the Cu content. Among the catalysts with different Cu contents, the catalyst with 20 wt.% of Cu represents the best compromise to obtain high catalytic activity and stability. On these bases, the catalytic performances seem to depend on both metallic Cu surface area and synergetic interactions between Cu and ZnO. The increase of the Al content enhances the homogeneity of the precursors, leading to a higher Cu dispersion and consequent better catalytic performances. The catalyst with 20 wt.% of Cu and a molar ratio M(II)/M(III) of 2 shows a high activity also at 250 °C and a good stability at middle temperature. Thus, it may be considered an optimum catalyst for the WGS reaction at middle temperature (about 300 °C). Finally, by replacing 50 % (as at. ratio) of Zn by Mg (which is not active in the WGS reaction), better physical properties were observed, although associate with poor catalytic performances. This result confirms the important role of ZnO on the catalytic performances, favoring synergetic interactions with metallic Cu.
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The last decade has witnessed an exponential growth of activities in the field of nanoscience and nanotechnology worldwide, driven both by the excitement of understanding new science and by the potential hope for applications and economic impacts. The largest activity in this field up to date has been in the synthesis and characterization of new materials consisting of particles with dimensions in the order of a few nanometers, so-called nanocrystalline materials. [1-8] Semiconductor nanomaterials such as III/V or II/VI compound semiconductors exhibit strong quantum confinement behavior in the size range from 1 to 10 nm. Therefore, preparation of high quality semiconductor nanocrystals has been a challenge for synthetic chemists, leading to the recent rapid progress in delivering a wide variety of semiconducting nanomaterials. Semiconductor nanocrystals, also called quantum dots, possess physical properties distinctly different from those of the bulk material. Typically, in the size range from 1 to 10 nm, when the particle size is changed, the band gap between the valence and the conduction band will change, too. In a simple approximation a particle in a box model has been used to describe the phenomenon[9]: at nanoscale dimensions the degenerate energy states of a semiconductor separate into discrete states and the system behaves like one big molecule. The size-dependent transformation of the energy levels of the particles is called “quantum size-effect”. Quantum confinement of both the electron and hole in all three dimensions leads to an increase in the effective bandgap of the material with decreasing crystallite size. Consequently, both the optical absorption and emission of semiconductor nanaocrystals shift to the blue (higher energies) as the size of the particles gets smaller. This color tuning is well documented for CdSe nanocrystals whose absorption and emission covers almost the whole visible spectral range. As particle sizes become smaller the ratio of surface atoms to those in the interior increases, which has a strong impact on particle properties, too. Prominent examples are the low melting point [8] and size/shape dependent pressure resistance [10] of semiconductor nanocrystals. Given the size dependence of particle properties, chemists and material scientists now have the unique opportunity to change the electronic and chemical properties of a material by simply controlling the particle size. In particular, CdSe nanocrystals have been widely investigated. Mainly due to their size-dependent optoelectronic properties [11, 12] and flexible chemical processibility [13], they have played a distinguished role for a number of seminal studies [11, 12, 14, 15]. Potential technical applications have been discussed, too. [8, 16-27] Improvement of the optoelectronic properties of semiconductor nanocrystals is still a prominent research topic. One of the most important approaches is fabricating composite type-I core-shell structures which exhibit improved properties, making them attractive from both a fundamental and a practical point of view. Overcoating of nanocrystallites with higher band gap inorganic materials has been shown to increase the photoluminescence quantum yields by eliminating surface nonradiative recombination sites. [28] Particles passivated with inorganic shells are more robust than nanocrystals covered by organic ligands only and have greater tolerance to processing conditions necessary for incorporation into solid state structures or for other applications. Some examples of core-shell nanocrystals reported earlier include CdS on CdSe [29], CdSe on CdS, [30], ZnS on CdS, [31] ZnS on CdSe[28, 32], ZnSe on CdSe [33] and CdS/HgS/CdS [34]. The characterization and preparation of a new core-shell structure, CdSe nanocrystals overcoated by different shells (CdS, ZnS), is presented in chapter 4. Type-I core-shell structures as mentioned above greatly improve the photoluminescence quantum yield and chemical and photochemical stability of nanocrystals. The emission wavelengths of type-I core/shell nanocrystals typically only shows a small red-shift when compared to the plain core nanocrystals. [30, 31, 35] In contrast to type-I core-shell nanocrystals, only few studies have been conducted on colloidal type-II core/shell structures [36-38] which are characterized by a staggered alignment of conduction and valence bands giving rise to a broad tunability of absorption and emission wavelengths, as was shown for CdTe/CdSe core-shell nanocrystals. [36] The emission of type-II core/shell nanocrystals mainly originates from the radiative recombination of electron-hole pairs across the core-shell interface leading to a long photoluminescence lifetime. Type-II core/shell nanocrystals are promising with respect to photoconduction or photovoltaic applications as has been discussed in the literature.[39] Novel type-II core-shell structures with ZnTe cores are reported in chapter 5. The recent progress in the shape control of semiconductor nanocrystals opens new fields of applications. For instance, rod shaped CdSe nanocrystals can enhance the photo-electro conversion efficiency of photovoltaic cells, [40, 41] and also allow for polarized emission in light emitting diodes. [42, 43] Shape control of anisotropic nanocrystals can be achieved by the use of surfactants, [44, 45] regular or inverse micelles as regulating agents, [46, 47] electrochemical processes, [48] template-assisted [49, 50] and solution-liquid-solution (SLS) growth mechnism. [51-53] Recently, formation of various CdSe nanocrystal shapes has been reported by the groups of Alivisatos [54] and Peng, [55] respectively. Furthermore, it has been reported by the group of Prasad [56] that noble metal nanoparticles can induce anisotropic growth of CdSe nanocrystals at lower temperatures than typically used in other methods for preparing anisotropic CdSe structures. Although several approaches for anisotropic crystal growth have been reported by now, developing new synthetic methods for the shape control of colloidal semiconductor nanocrystals remains an important goal. Accordingly, we have attempted to utilize a crystal phase control approach for the controllable synthesis of colloidal ZnE/CdSe (E = S, Se, Te) heterostructures in a variety of morphologies. The complex heterostructures obtained are presented in chapter 6. The unique optical properties of nanocrystals make them appealing as in vivo and in vitro fluorophores in a variety of biological and chemical investigations, in which traditional fluorescence labels based on organic molecules fall short of providing long-term stability and simultaneous detection of multiple emission colours [References]. The ability to prepare water soluble nanocrystals with high stability and quantum yield has led to promising applications in cellular labeling, [57, 58] deep-tissue imaging, [59, 60] and assay labeling [61, 62]. Furthermore, appropriately solubilized nanocrystals have been used as donors in fluorescence resonance energy transfer (FRET) couples. [63-65] Despite recent progress, much work still needs to be done to achieve reproducible and robust surface functionalization and develop flexible (bio-) conjugation techniques. Based on multi-shell CdSe nanocrystals, several new solubilization and ligand exchange protocols have been developed which are presented in chapter 7. The organization of this thesis is as follows: A short overview describing synthesis and properties of CdSe nanocrystals is given in chapter 2. Chapter 3 is the experimental part providing some background information about the optical and analytical methods used in this thesis. The following chapters report the results of this work: synthesis and characterization of type-I multi-shell and type-II core/shell nanocrystals are described in chapter 4 and chapter 5, respectively. In chapter 6, a high–yield synthesis of various CdSe architectures by crystal phase control is reported. Experiments about surface modification of nanocrystals are described in chapter 7. At last, a short summary of the results is given in chapter 8.
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Blue straggler stars (BSSs) are brighter and bluer (hotter) than the main-sequence (MS) turnoff and they are known to be more massive than MS stars.Two main scenarios for their formation have been proposed:collision-induced stellar mergers (COL-BSSs),or mass-transfer in binary systems (MT-BSSs).Depleted surface abundances of C and O are expected for MT-BSSs,whereas no chemical anomalies are predicted for COL-BSSs.Both MT- and COL-BSSs should rotate fast, but braking mechanisms may intervene with efficiencies and time-scales not well known yet,thus preventing a clear prediction of the expected rotational velocities.Within this context,an extensive survey is ongoing by using the multi-object spectrograph FLAMES@VLT,with the aim to obtain abundance patterns and rotational velocities for representative samples of BSSs in several Galactic GCs.A sub-population of CO-depleted BSSs has been identified in 47 Tuc,with only one fast rotating star detected.For this PhD Thesis work I analyzed FLAMES spectra of more than 130 BSSs in four GCs:M4,NGC 6397,M30 and ω Centauri.This is the largest sample of BSSs spectroscopically investigated so far.Hints of CO depletion have been observed in only 4-5 cases (in M30 and ω Centauri),suggesting either that the majority of BSSs have a collisional origin,or that the CO-depletion is a transient phenomenon.Unfortunately,no conclusions in terms of formation mechanism could be drawn in a large number of cases,because of the effects of radiative levitation. Remarkably,however,this is the first time that evidence of radiative levitation is found in BSSs hotter than 8200 K.Finally, we also discovered the largest fractions of fast rotating BSSs ever observed in any GCs:40% in M4 and 30% in ω Centauri.While not solving the problem of BSS formation,these results provide invaluable information about the BSS physical properties,which is crucial to build realistic models of their evolution.
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Negli ultimi anni l’interesse nei confronti dell’H2 è cresciuto notevolmente per l’aumento della richiesta energetica mondiale. Uno dei processi più importanti per la produzione di H2 utilizza la reazione di Water-Gas Shift (WGS) per il trattamento delle correnti in uscita dai processi di steam reforming o di ossidazione parziale catalitica. CO + H2O CO2 + H2 ∆H0298 = -41,2 KJ/mol Sono quindi stati sviluppati sistemi catalitici attivi nella reazione di WGS a media temperatura (circa 300 °C). Partendo da sistemi catalitici a base di Cu/Zn/Al, ottenuti da precursori idrotalcitici e sviluppati in lavori di tesi precedenti, sono state effettuate modifiche nella composizione al fine di aumentarne l’attività e la stabilità. L’aggiunta di piccole quantità di Mg ha un effetto positivo sull’attività dei sistemi catalitici, con effetti più evidenti a 250 °C. Tuttavia, l’aumento del contenuto di Mg, sebbene migliori le proprietà fisiche del catalizzatore (area superficiale e dispersione del Cu) sia del campione calcinato che di quello scaricato dopo reazione, peggiora drasticamente l’attività catalitica. L’aggiunta di piccole quantità di Mg sembra portare alla stabilizzazione della specie attiva Cu+ e promuovere un meccanismo redox superficiale (Cu0 e Cu+). E’ possibile correlare la conversione del CO con il rapporto ZnO/Cu, confermando il ruolo nella reazione di WGS dell’interazione Cu0/ZnO libero. La sostituzione di Mg con Ba comporta un miglioramento delle prestazioni catalitiche, in particolare nelle condizioni MTS (300 °C), suggerendo una più facile dissociazione dell’acqua legata alla stabilizzazione degli ossidrili da parte dei siti basici. È però accompagnato da una diminuzione della stabilità nelle condizioni di reazione. L’aggiunta di piccole quantità di La, Ce o Zr (con un rapporto Al/R = 50 mol/mol) incrementa la stabilità termica, sia in termini di proprietà fisiche che di attività catalitica. A seguito dei cicli termici di invecchiamento accelerato, infatti, non si riscontrano importanti diminuzioni di attività catalitica, evidenziando un’elevata stabilità della fase attiva.
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Per massimizzare la quantità di H2 nel gas di sintesi ottenuto dal processo di Steam Reforming (SR) si utilizza la reazione di Water Gas Shift (WGS): CO + H2O ⇆ CO2 + H2 ∆H0298 = - 41,2 KJ/mol Sulla base di sistemi catalitici Cu/Zn/Al si è cercato di modificarne la composizione per ottenere catalizzatori attivi e stabili in un intervallo di temperatura tra 350-450 °C, (High Temperature Shift o HTS), al fine di sostituire i tradizionali sistemi a base di Fe/Cr, in relazione alle limitazioni ambientali all’utilizzo del Cr e per poter operare con valori inferiori del rapporto S/DG. Si sono inoltre studiate le caratteristiche dei catalizzatori e le condizioni di reazione che favoriscono la produzione di metilammine ed alcoli nel processo a temperature intermedie, tra 300-350 °C (Middle Temperature Shift o MTS), in relazione alla disattivazione che questi composti comportano nel processo di SR a seguito del riciclo della fase acquosa dal reattore di WGS.
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This thesis reports on the realization, characterization and analysis of ultracold bosonic and fermionic atoms in three-dimensional optical lattice potentials. Ultracold quantum gases in optical lattices can be regarded as ideal model systems to investigate quantum many-body physics. In this work interacting ensembles of bosonic 87Rb and fermionic 40K atoms are employed to study equilibrium phases and nonequilibrium dynamics. The investigations are enabled by a versatile experimental setup, whose core feature is a blue-detuned optical lattice that is combined with Feshbach resonances and a red-detuned dipole trap to allow for independent control of tunneling, interactions and external confinement. The Fermi-Hubbard model, which plays a central role in the theoretical description of strongly correlated electrons, is experimentally realized by loading interacting fermionic spin mixtures into the optical lattice. Using phase-contrast imaging the in-situ size of the atomic density distribution is measured, which allows to extract the global compressibility of the many-body state as a function of interaction and external confinement. Thereby, metallic and insulating phases are clearly identified. At strongly repulsive interaction, a vanishing compressibility and suppression of doubly occupied lattice sites signal the emergence of a fermionic Mott insulator. In a second series of experiments interaction effects in bosonic lattice quantum gases are analyzed. Typically, interactions between microscopic particles are described as two-body interactions. As such they are also contained in the single-band Bose-Hubbard model. However, our measurements demonstrate the presence of multi-body interactions that effectively emerge via virtual transitions of atoms to higher lattice bands. These findings are enabled by the development of a novel atom optical measurement technique: In quantum phase revival spectroscopy periodic collapse and revival dynamics of the bosonic matter wave field are induced. The frequencies of the dynamics are directly related to the on-site interaction energies of atomic Fock states and can be read out with high precision. The third part of this work deals with mixtures of bosons and fermions in optical lattices, in which the interspecies interactions are accurately controlled by means of a Feshbach resonance. Studies of the equilibrium phases show that the bosonic superfluid to Mott insulator transition is shifted towards lower lattice depths when bosons and fermions interact attractively. This observation is further analyzed by applying quantum phase revival spectroscopy to few-body systems consisting of a single fermion and a coherent bosonic field on individual lattice sites. In addition to the direct measurement of Bose-Fermi interaction energies, Bose-Bose interactions are proven to be modified by the presence of a fermion. This renormalization of bosonic interaction energies can explain the shift of the Mott insulator transition. The experiments of this thesis lay important foundations for future studies of quantum magnetism with fermionic spin mixtures as well as for the realization of complex quantum phases with Bose-Fermi mixtures. They furthermore point towards physics that reaches beyond the single-band Hubbard model.
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Passive acoustic data have been collected using HARPs (High-frequency Acoustic Recording Packages) and were used to assess (1) the seasonality of blue whale D calls in the Southern California Bight, (2) their interannual abundance during 2007-2012 and (3) their diel variation. This goal has been achieved running the GPL (Generalized Power-Law) automated detector. (1) Blue whale D calls were detected in the Southern California Bight from May through November with a peak in July, even though few detections were from December to April as well. A key predictor for blue whale distribution and movement in the California Current region has been identified with zooplankton aggregations, paying a particular attention to those euphausiid species, such as E. pacifica and T. spinifera, which are blue whale favorite krill. The Southern California Bight experiences seasonal upwelling, resulting in an increase of productivity and prey availability. The summer and early fall have been marked as the most favorable periods. This supports the presence of blue whales in the area at that time, supposing these marine mammals exploit the region as a feeding ground. (2) As to the interannual abundance during 2007-2012, I found a large variability. I observed a great increase of vocalizations in 2007 and 2010, whereas a decrease was shown in the other years, which is well marked in 2009. It is my belief that these fluctuations in abundance of D calls detections through the deployed period are due to the alternation of El Nino and La Nina events, which occurred in those years. (3) The assessment of the daily timing of D calls production shows that D calls are more abundant during the day than during the night with a peak at 12:00 and 13:00. Assuming that D calling is associated with feeding, the daily pattern of D calls may be linked to the prey availability. E. pacifica and T. spinifera are among those species of krill which undertake daily vertical migrations, remaining at depth during the day and slowly coming up towards the surface at night. Because of some anatomical arrangements, these euphausiids are very sensitive to the light. Given that we believe D calls have a social function, I hypothesize that blue whales may recognize the hours at the highest solar incidence as the best moment of the day in terms of prey availability, exploiting this time window to advert their conspecifics.
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Increasing knowledge on the endocrine mechanisms that regulate feeding and growth in cultured fish can contribute to make improvement in fish holding conditions and feeding strategies, supporting the development of new techniques that could ameliorate feeding, food conversion efficiency and growth in aquaculture practice. The main objective of this study was to investigate how daily mRNA expression of three specific anorexigenic hormones, i.e. the corticotropin-releasing hormone (CRH) and the paralogues α- and β- proopiomelanocortin (POMC), is modulated by different photoperiods, light spectra and feeding regimes, in both adult and larvae of Solea senegalensis. In addition, as Senegalese sole exhibits a shift from diurnal to nocturnal in locomotor activity and feeding habits during metamorphic process, we tried to elucidate if this shift is accompanied by relevant daily variations in the expression of these anorexigenic hormones before, during and after the completion of metamorphosis. In order to reach this main objective, three main experiments were developed. In a first experiment, adults were reared under LD (12 h light: 12h dark) cycle and fed at mid-light (ML), mid-dark (MD) and at random (RND). In a second experiment, adult specimens were reared in constant darkness (DD) and fed at subjective mid-light (sML) or at RND. Larvae of Senegalese sole were reared under LD cycle with white, blue or red light for 40 days. Our results show an independence of crh mRNA expression from the feeding time and suggest an endogenous control of crh expression in sole. Both pomc paralogues showed significant daily rhythms under LD conditions. The rhythms were maintained or were even more robust under DD conditions for pomc_a, but were completely abolished for pomc_b. Our results indicate an endogenous control of pomc_a expression by the molecular clock in telencephalon and diencephalon, but not in the pituitary gland. Our findings confirm for the first time the significant influence that ambient lighting has on larval growth and development in Senegalese sole, revealing an important effect of light spectra upon functional elements of this species. Our results also emphasize the importance of maintaining cycling light-dark conditions of the adequate wavelengths in aquaculture practices during early development of sole.
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L’H2 è un vettore energetico di elevato interesse, utilizzato nell’industria chimica per la produzione di NH3 e CH3OH, oltre che per le reazioni di idrogenazione ed HDS. Un importante processo nella produzione di H2 è la reazione di Water Gas Shift (WGS), usata nel trattamento delle correnti uscenti dal reattore di Steam Reforming (SR) del metano: CO + H2O CO2 + H2 ∆H0298K = -41,2 KJ/mol. Sulla base di precedenti lavori, sono stati sviluppati nuovi catalizzatori per la reazione WGS ad alta temperatura (HTS), alternativi ai tradizionali sistemi a base di Fe/Cr, in considerazione dei vincoli economici (elevati valori del rapporto vapore/gas secco o S/DG) ed ambientali (formazione di CrVI) di questi sistemi. Partendo da sistemi Cu/Zn/Al con un basso contenuto di rame, ottenuti da precursori tipo idrotalcite (HT), stato studiato l’effetto dell’aggiunta di piccole quantità di alcuni promotori sull’attività e stabilità dei catalizzatori ottenuti, osservando un effetto positivo sulle caratteristiche fisiche, come l’aumento dell’area superficiale e della dispersione della fase attiva. I campioni contenenti i promotori erano inoltre caratterizzati da una maggiore stabilità termica e, in alcuni casi, da un’attività catalitica superiore a quella del catalizzatore di riferimento privo di promotori. L’aggiunta di piccole quantità di alcali alla formulazione con la migliore attività portava ad un ulteriore aumento di attività e di stabilità, attribuibile ad una minore formazione di coke sulla superficie. I sistemi più interessanti potevano operare anche a bassi valori del rapporto S/DG, interessanti dal punto di vista industriale. Lo studio dell’adsorbimento di CO mediante FT-IR ha permesso di ipotizzare la possibile natura della fase attiva nei sistemi. Infine, lo studio è stato esteso a sistemi per la reazione di WGS a media temperatura (MTS), osservando anche in questo caso un positivo effetto legato all’aggiunta di promotori, con un aumento dell’attività catalitica e della stabilità con il tempo di reazione.
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Le Blue Straggler Stars (BSS) sono la popolazione di oggetti esotici piu' comune e numerosa negli ammassi globulari. Nel diagramma colore-magnitudine le BSS definiscono una sequenza più brillante e blu del punto di turn-off della Sequenza Principale, simulando una popolazione più giovane delle stelle dell'ammasso. Osservazioni hanno dimostrato che le BSS hanno una massa significativamente più grande (1.2-1.7 Msun) di quella delle stelle di un ammasso globulare. Per questa proprietà, la distribuzione radiale delle BSS e' un utile strumento per tracciare empiricamente lo stato di evoluzione dinamica degli ammassi stellari. Il lavoro di tesi si è concentrato sullo studio della popolazione di BSS di due ammassi globulari della Grande Nube di Magellano: NGC2257 e NGC1754. Applicando metodi di indagine già usati per sistemi stellari della Via Lattea, abbiamo derivato le eta' dinamiche di questi due sistemi e le abbiamo confrontate con stime teoriche.