Effects of Nb doping on the TiO2 anatase-to-rutile phase transition

We study the influence of Nb doping on the TiO2 anatase-to-rutile phase transition, using combined transmission electron microscopy, Raman spectroscopy, x-ray diffraction and selected area electron diffraction analysis. This approach enabled anatase-to-rutile phase transition hindering to be clearly observed for low Nb-doped TiO2 samples. Moreover, there was clear grain growth inhibition in the samples containing Nb. The use of high resolution transmission electron microscopy with our samples provides an innovative perspective compared with previous research on this issue. Our analysis shows that niobium is segregated from the anatase structure before and during the phase transformation, leading to the formation of NbO nanoclusters on the surface of the TiO2 rutile nanoparticles.

Influence of average size and interface passivation on the spectral emission of Si nanocrystals embedded in SiO2

The correlation between the structural (average size and density) and optoelectronic properties [band gap and photoluminescence (PL)] of Si nanocrystals embedded in SiO2 is among the essential factors in understanding their emission mechanism. This correlation has been difficult to establish in the past due to the lack of reliable methods for measuring the size distribution of nanocrystals from electron microscopy, mainly because of the insufficient contrast between Si and SiO2. With this aim, we have recently developed a successful method for imaging Si nanocrystals in SiO2 matrices. This is done by using high-resolution electron microscopy in conjunction with conventional electron microscopy in dark field conditions. Then, by varying the time of annealing in a large time scale we have been able to track the nucleation, pure growth, and ripening stages of the nanocrystal population. The nucleation and pure growth stages are almost completed after a few minutes of annealing time at 1100°C in N2 and afterward the ensemble undergoes an asymptotic ripening process. In contrast, the PL intensity steadily increases and reaches saturation after 3-4 h of annealing at 1100°C. Forming gas postannealing considerably enhances the PL intensity but only for samples annealed previously in less time than that needed for PL saturation. The effects of forming gas are reversible and do not modify the spectral shape of the PL emission. The PL intensity shows at all times an inverse correlation with the amount of Pb paramagnetic centers at the Si-SiO2 nanocrystal-matrix interfaces, which have been measured by electron spin resonance. Consequently, the Pb centers or other centers associated with them are interfacial nonradiative channels for recombination and the emission yield largely depends on the interface passivation. We have correlated as well the average size of the nanocrystals with their optical band gap and PL emission energy. The band gap and emission energy shift to the blue as the nanocrystal size shrinks, in agreement with models based on quantum confinement. As a main result, we have found that the Stokes shift is independent of the average size of nanocrystals and has a constant value of 0.26±0.03 eV, which is almost twice the energy of the Si¿O vibration. This finding suggests that among the possible channels for radiative recombination, the dominant one for Si nanocrystals embedded in SiO2 is a fundamental transition spatially located at the Si¿SiO2 interface with the assistance of a local Si-O vibration.

Diffractive J/Psi photoproduction in a dual model

J/psi photoproduction is studied in the framework of the analytic S-matrix theory. The differential and integrated elastic cross sections for J/psi photoproduction are calculated from a dual amplitude with Mandelstam analyticity. It is argued that, at low energies, the background, which is the low-energy equivalent of the high-energy diffraction, replaces the Pomeron exchange. The onset of the high-energy Pomeron dominance is estimated from the fits to the data.

Polymorphous Si thin films from radio frequency plasmas of SiH4 diluted in Ar: A study by transmission electron microscopy and Raman spectroscopy

In this study, we present a detailed structural characterization by means of transmission electron microscopy and Raman spectroscopy of polymorphous silicon (pm-Si:H) thin films deposited using radio-frequency dust-forming plasmas of SiH4 diluted in Ar. Square-wave modulation of the plasma and gas temperature was varied to obtain films with different nanostructures. Transmission electron microscopy and electron diffraction have shown the presence of Si crystallites of around 2 nm in the pm-Si:H films, which are related to the nanoparticles formed in the plasma gas phase coming from their different growth stages, named particle nucleation and coagulation. Raman scattering has proved the role of the film nanostructure in the crystallization process induced ¿in situ¿ by laser heating.

Evidence for oxygen-island formation on Al(111): Cluster-model theory and x-ray photoelectron spectroscopy

The O 1s x-ray photoelectron spectroscopy spectrum for Al(111)/O at 300 K shows two components whose behavior as a function of time and variation of detection angle are consistent with either (a) a surface species represented by the higher binding-energy (BE) component and a subsurface species represented by the lower BE component, or (b) small close-packed oxygen islands with the interior atoms represented by the lower BE component and the perimeter atoms by the higher BE component. We have modeled both situations using ab initio Hartree-Fock wave functions for clusters of Al and O atoms. For an O atom in a threefold site, it was found that a below-surface position gave a higher O 1s BE than an above-surface position, incompatible with interpretation (a). This change in the O 1s BE could arise because the bond for O to Al may have a more covalent character when the O is below the surface than when it is above the surface. We present evidence consistent with this view. An O adatom island with all the O atoms in threefold sites gives calculated O 1s BE's which are significantly higher for the perimeter O atoms. Further, the results for an isolated O island without the Al substrate present also give higher BE¿s for the perimeter atoms. Both these results are consistent with interpretation (b). Published scanning-tunneling-microscopy data supports the suggestion that the chemisorbed state consists of small, close-packed islands, whereas the presence of two vibrational modes in high-resolution electron-energy-loss spectroscopy data has been interpreted as representing surface and subsurface oxygen atoms. In light of the present results, we suggest that a vibrational interpretation in terms of interior and perimeter adatoms should be considered.

Performance and hormonal profile in broiler chickens fed with different energy levels during post restriction period

The aim of this work was to investigate the influence of diet energy level on performance and hormonal profiles of broilers during post restriction period. It was a split-plot experiment, and the main treatments were in a 2x2 factorial scheme. Birds were fed restricted to 30% of the ad libitum intake, from 7 to 14 days of age. After the restriction period, birds were fed ad libitum with diets containing low (2,900 kcal ME/kg) or high (3,200 kcal ME/kg) energy until 49 days of age. Broilers fed with high energy ration showed lower feed intake and better feed conversion and decreased carcass protein; however, abdominal fat pad, and total carcass fat were not affected by ration energy levels or feeding program. Neither diet energy level nor feed restriction program changed body weight at 49 days. The profile of insulin-like growth factor-1 (IGF-1) was reduced during the feed restriction period, but increased at refeeding period. Feeding program and ration energy level did not affect T3, T4 and growth hormone serum concentrations. Feed restriction at 30% of ad libitum intake is not enough to promote changes on carcass quality, related to fat deposition, and on metabolic hormone levels, except IGF-1 seric level that has rapid increase after feed restriction.

Characterization of polyphosphate synthesis by isolated yeast vacuoles

Polyphosphate (iPOP) is a linear polymer of orthophosphate units linked together by high energy phosphoanhydride bonds. It is found in all organisms, localized in organelles called acidocalcisomes and ranges from a few to few hundred monomers in length. iPOP has been found to play a vast array of roles in all organisms, including phosphate and energy metabolism, regulation of enzymes, virulence, pathogenicity, bone remodelling and blood clotting, among many others. Recently it was found that iPOP levels were increased in myeloma cells. The growing interest in iPOP in human cell lines makes it an interesting molecule to study. However, not much is known about its metabolism in eukaryotes. Acidocalcisomes are electron dense, acidic organelles that belong to the group of Lysosome Related Organelles (LROs). The conservation of acidocalcisomes among all kingdoms of life is suggestive of their important roles for the organisms. However, they are difficult to analyse because of limited biochemical tools for investigation. Yeast vacuoles present remarkable similarities to acidocalcisomes in terms of their physiological and structural features, including synthesis and storage of iPOP, which make them an ideal candidate to study biological processes which are shared between vacuoles and acidocalcisomes. The availability of tools for genetic manipulation and isolation of vacuoles makes yeast a candidate of choice for the characterization of iPOP synthesis in eukaryotes. Our group has identified the Vacuolar Transporter Chaperone (VTC) complex as iPOP polymerase and identified the catalytic subunit (Vtc4). The goal of my study was to characterize the process of iPOP synthesis by isolated vacuoles and to reconstitute iPOP synthesis in liposomes. The first step was to develop a method for monitoring iPOP by isolated vacuoles over time and comparing it with previously known methods. Next, a detailed characterization was performed to determine the modulators of the process, both for intact as well as solubilized vacuoles. Finally, attempts were made to purify the VTC complex and reconstitute it in liposomes. A parallel line of study was the translocation and storage of synthesized iPOP in the lumen of the vacuoles. As a result of this study, it is possible to determine distinct pools of iPOP- inside and outside the vacuolar lumen. Additionally, I establish that the vacuolar lysate withstands harsh steps during reconstitution on liposomes and retains iPOP synthesizing activity. The next steps will be purification of the intact VTC complex and its structure determination by cryo-electron microscopy. - Les organismes vivants sont composés d'une ou plusieurs cellules responsables des processus biologiques élémentaires tels que la digestion, la respiration, la synthèse et la reproduction. Leur environnement interne est en équilibre et ils réalisent un très grand nombre de réactions chimiques et biochimiques pour maintenir cet équilibre. A différents compartiments cellulaires, ou organelles, sont attribuées des tâches spécifiques pour maintenir les cellules en vie. L'étude de ces fonctions permet une meilleure compréhension de la vie et des organismes vivants. De nombreux processus sont bien connus et caractérisés mais d'autres nécessitent encore des investigations détaillées. L'un de ces processus est le métabolisme des polyphosphates. Ces molécules sont des polymères linéaires de phosphate inorganique dont la taille peut varier de quelques dizaines à quelques centaines d'unités élémentaires. Ils sont présents dans tous les organismes, des bactéries à l'homme. Ils sont localisés principalement dans des compartiments cellulaires appelés acidocalcisomes, des organelles acides observés en microscopie électronique comme des structures denses aux électrons. Les polyphosphates jouent un rôle important dans le stockage et le métabolisme de l'énergie, la réponse au stress, la virulence, la pathogénicité et la résistance aux drogues. Chez l'homme, ils sont impliqués dans la coagulation du sang et le remodelage osseux. De nouvelles fonctions biologiques des polyphosphates sont encore découvertes, ce qui accroît l'intérêt des chercheurs pour ces molécules. Bien que des progrès considérables ont été réalisés afin de comprendre la fonction des polyphosphates chez les bactéries, ce qui concerne la synthèse, le stockage et la dégradation des polyphosphates chez les eucaryotes est mal connu. Les vacuoles de la levure Saccharomyces cerevisiae sont similaires aux acidocalcisomes des organismes supérieurs en termes de structure et de fonction. Les acidocalcisomes sont difficiles à étudier car il n'existe que peu d'outils génétiques et biochimiques qui permettent leur caractérisation. En revanche, les vacuoles peuvent être aisément isolées des cellules vivantes et manipulées génétiquement. Les vacuoles comme les acidocalcisomes synthétisent et stockent les polyphosphates. Ainsi, les découvertes faites grâce aux vacuoles de levures peuvent être extrapolées aux acidocalcisomes des organismes supérieurs. Le but de mon projet était de caractériser la synthèse des polyphosphates par des vacuoles isolées. Au cours de mon travail de thèse, j'ai mis au point une méthode de mesure de la synthèse des polyphosphates par des organelles purifés. Ensuite, j'ai identifié des composés qui modulent la réaction enzymatique lorsque celle-ci a lieu dans la vacuole ou après solubilisation de l'organelle. J'ai ainsi pu mettre en évidence deux groupes distincts de polyphosphates dans le système : ceux au-dehors de la vacuole et ceux en-dedans de l'organelle. Cette observation suggère donc très fortement que les vacuoles non seulement synthétisent les polyphosphates mais aussi transfère les molécules synthétisées de l'extérieur vers l'intérieur de l'organelle. Il est très vraisemblable que les vacuoles régulent le renouvellement des polyphosphates qu'elles conservent, en réponse à des signaux cellulaires. Des essais de purification de l'enzyme synthétisant les polyphosphates ainsi que sa reconstitution dans des liposomes ont également été entrepris. Ainsi, mon travail présente de nouveaux aspects de la synthèse des polyphosphates chez les eucaryotes et les résultats devraient encourager l'élucidation de mécanismes similaires chez les organismes supérieurs. - Les polyphosphates (iPOP) sont des polymères linéaires de phosphates inorganiques liés par des liaisons phosphoanhydres de haute énergie. Ces molécules sont présentes dans tous les organismes et localisées dans des compartiments cellulaires appelés acidocalcisomes. Elles varient en taille de quelques dizaines à quelques centaines d'unités phosphate. Des fonctions nombreuses et variées ont été attribuées aux iPOP dont un rôle dans les métabolismes de l'énergie et du phosphate, dans la régulation d'activités enzymatiques, la virulence, la pathogénicité, le remodelage osseux et la coagulation sanguine. Il a récemment été montré que les cellules de myélome contiennent une grande quantité de iPOP. Il y donc un intérêt croissant pour les iPOP dans les lignées cellulaires humaines. Cependant, très peu d'informations sur le métabolisme des iPOP chez les eucaryotes sont disponibles. Les acidocalcisomes sont des compartiments acides et denses aux électrons. Ils font partie du groupe des organelles similaires aux lysosomes (LROs pour Lysosome Related Organelles). Le fait que les acidocalcisomes soient conservés dans tous les règnes du vivant montrent l'importance de ces compartiments pour les organismes. Cependant, l'analyse de ces organelles est rendue difficile par l'existence d'un nombre limité d'outils biochimiques permettant leur caractérisation. Les vacuoles de levures possèdent des aspects structuraux et physiologiques très similaires à ceux des acidocalcisomes. Par exemple, ils synthétisent et gardent en réserve les iPOP. Ceci fait des vacuoles de levure un modèle idéal pour l'étude de processus biologiques conservés chez les vacuoles et les acidocalcisomes. De plus, la levure est un organisme de choix pour l'étude de la synthèse des iPOP compte-tenu de l'existence de nombreux outils génétiques et la possibilité d'isoler des vacuoles fonctionnelles. Notre groupe a identifié le complexe VTC (Vacuole transporter Chaperone) comme étant responsable de la synthèse des iPOP et la sous-unité Vtc4p comme celle possédant l'activité catalytique. L'objectif de cette étude était de caractériser le processus de synthèse des iPOP en utilisant des vacuoles isolées et de reconstituer la synthèse des iPOP dans des liposomes. La première étape a consisté en la mise au point d'un dosage permettant la mesure de la quantité de iPOP synthétisés par les organelles isolés en fonction du temps. Cette nouvelle méthode a été comparée aux méthodes décrites précédemment dans la littérature. Ensuite, la caractérisation détaillée du processus a permis d'identifier des composés modulateurs de la réaction à la fois pour des vacuoles intactes et des vacuoles solubilisées. Enfin, des essais de purification du complexe VTC et sa reconstitution dans des liposomes ont été entrepris. De façon parallèle, une étude sur la translocation et le stockage des iPOP dans le lumen des vacuoles a été menée. Il a ainsi été possible de mettre en évidence différents groupes de iPOP : les iPOP localisés à l'intérieur et ceux localisés à l'extérieur des vacuoles isolées. De plus, nous avons observé que le lysat vacuolaire n'est pas détérioré par les étapes de reconstitution dans les liposomes et conserve l'activité de synthèse des iPOP. Les prochaines étapes consisteront en la purification du complexe intact et de la détermination de sa structure par cryo-microscopie électronique.

Forecasting the Earth"s radiation belts and modeling solar energetic particle events: Recent results from SPACECAST

High-energy charged particles in the van Allen radiation belts and in solar energetic particle events can damage satellites on orbit leading to malfunctions and loss of satellite service. Here we describe some recent results from the SPACECAST project on modelling and forecasting the radiation belts, and modelling solar energetic particle events. We describe the SPACECAST forecasting system that uses physical models that include wave-particle interactions to forecast the electron radiation belts up to 3 h ahead. We show that the forecasts were able to reproduce the >2 MeV electron flux at GOES 13 during the moderate storm of 7-8 October 2012, and the period following a fast solar wind stream on 25-26 October 2012 to within a factor of 5 or so. At lower energies of 10- a few 100 keV we show that the electron flux at geostationary orbit depends sensitively on the high-energy tail of the source distribution near 10 RE on the nightside of the Earth, and that the source is best represented by a kappa distribution. We present a new model of whistler mode chorus determined from multiple satellite measurements which shows that the effects of wave-particle interactions beyond geostationary orbit are likely to be very significant. We also present radial diffusion coefficients calculated from satellite data at geostationary orbit which vary with Kp by over four orders of magnitude. We describe a new automated method to determine the position at the shock that is magnetically connected to the Earth for modelling solar energetic particle events and which takes into account entropy, and predict the form of the mean free path in the foreshock, and particle injection efficiency at the shock from analytical theory which can be tested in simulations.

Forecasting the Earth"s radiation belts and modeling solar energetic particle events: Recent results from SPACECAST

High-energy charged particles in the van Allen radiation belts and in solar energetic particle events can damage satellites on orbit leading to malfunctions and loss of satellite service. Here we describe some recent results from the SPACECAST project on modelling and forecasting the radiation belts, and modelling solar energetic particle events. We describe the SPACECAST forecasting system that uses physical models that include wave-particle interactions to forecast the electron radiation belts up to 3 h ahead. We show that the forecasts were able to reproduce the >2 MeV electron flux at GOES 13 during the moderate storm of 7-8 October 2012, and the period following a fast solar wind stream on 25-26 October 2012 to within a factor of 5 or so. At lower energies of 10- a few 100 keV we show that the electron flux at geostationary orbit depends sensitively on the high-energy tail of the source distribution near 10 RE on the nightside of the Earth, and that the source is best represented by a kappa distribution. We present a new model of whistler mode chorus determined from multiple satellite measurements which shows that the effects of wave-particle interactions beyond geostationary orbit are likely to be very significant. We also present radial diffusion coefficients calculated from satellite data at geostationary orbit which vary with Kp by over four orders of magnitude. We describe a new automated method to determine the position at the shock that is magnetically connected to the Earth for modelling solar energetic particle events and which takes into account entropy, and predict the form of the mean free path in the foreshock, and particle injection efficiency at the shock from analytical theory which can be tested in simulations.

A high-mobility, low-cost phenotype defines human effector-memory CD8+ T cells.

T cells move randomly ("random-walk"), a characteristic thought to be integral to their function. Using migration assays and time-lapse microscopy, we found that CD8+ T cells lacking the lymph node homing receptors CCR7 and CD62L migrate more efficiently in transwell assays, and that these same cells are characterized by a high frequency of cells exhibiting random crawling activity under culture conditions mimicking the interstitial/extravascular milieu, but not when examined on endothelial cells. To assess the energy efficiency of cells crawling at a high frequency, we measured mRNA expression of genes key to mitochondrial energy metabolism (peroxisome proliferator-activated receptor gamma coactivator 1beta [PGC-1beta], estrogen-related receptor alpha [ERRalpha], cytochrome C, ATP synthase, and the uncoupling proteins [UCPs] UCP-2 and -3), quantified ATP contents, and performed calorimetric analyses. Together these assays indicated a high energy efficiency of the high crawling frequency CD8+ T-cell population, and identified differentially regulated heat production among nonlymphoid versus lymphoid homing CD8+ T cells.

Fabrication and characterization of silicon position sensitive particle detectors

Position sensitive particle detectors are needed in high energy physics research. This thesis describes the development of fabrication processes and characterization techniques of silicon microstrip detectors used in the work for searching elementary particles in the European center for nuclear research, CERN. The detectors give an electrical signal along the particles trajectory after a collision in the particle accelerator. The trajectories give information about the nature of the particle in the struggle to reveal the structure of the matter and the universe. Detectors made of semiconductors have a better position resolution than conventional wire chamber detectors. Silicon semiconductor is overwhelmingly used as a detector material because of its cheapness and standard usage in integrated circuit industry. After a short spread sheet analysis of the basic building block of radiation detectors, the pn junction, the operation of a silicon radiation detector is discussed in general. The microstrip detector is then introduced and the detailed structure of a double-sided ac-coupled strip detector revealed. The fabrication aspects of strip detectors are discussedstarting from the process development and general principles ending up to the description of the double-sided ac-coupled strip detector process. Recombination and generation lifetime measurements in radiation detectors are discussed shortly. The results of electrical tests, ie. measuring the leakage currents and bias resistors, are displayed. The beam test setups and the results, the signal to noise ratio and the position accuracy, are then described. It was found out in earlier research that a heavy irradiation changes the properties of radiation detectors dramatically. A scanning electron microscope method was developed to measure the electric potential and field inside irradiated detectorsto see how a high radiation fluence changes them. The method and the most important results are discussed shortly.

The first SEPServer event catalogue 68-MeV solar proton events observed at 1 AU in 1996-2010

SEPServer is a three-year collaborative project funded by the seventh framework programme (FP7-SPACE) of the European Union. The objective of the project is to provide access to state-of-the-art observations and analysis tools for the scientific community on solar energetic particle (SEP) events and related electromagnetic (EM) emissions. The project will eventually lead to better understanding of the particle acceleration and transport processes at the Sun and in the inner heliosphere. These processes lead to SEP events that form one of the key elements of space weather. In this paper we present the first results from the systematic analysis work performed on the following datasets: SOHO/ERNE, SOHO/EPHIN, ACE/EPAM, Wind/WAVES and GOES X-rays. A catalogue of SEP events at 1 AU, with complete coverage over solar cycle 23, based on high-energy (~68-MeV) protons from SOHO/ERNE and electron recordings of the events by SOHO/EPHIN and ACE/EPAM are presented. A total of 115 energetic particle events have been identified and analysed using velocity dispersion analysis (VDA) for protons and time-shifting analysis (TSA) for electrons and protons in order to infer the SEP release times at the Sun. EM observations during the times of the SEP event onset have been gathered and compared to the release time estimates of particles. Data from those events that occurred during the European day-time, i.e., those that also have observations from ground-based observatories included in SEPServer, are listed and a preliminary analysis of their associations is presented. We find that VDA results for protons can be a useful tool for the analysis of proton release times, but if the derived proton path length is out of a range of 1 AU < s[3 AU, the result of the analysis may be compromised, as indicated by the anti-correlation of the derived path length and release time delay from the asso ciated X-ray flare. The average path length derived from VDA is about 1.9 times the nominal length of the spiral magnetic field line. This implies that the path length of first-arriving MeV to deka-MeV protons is affected by interplanetary scattering. TSA of near-relativistic electrons results in a release time that shows significant scatter with respect to the EM emissions but with a trend of being delayed more with increasing distance between the flare and the nominal footpoint of the Earth-connected field line.

Spectral energy distribution of the gamma-ray microquasar LS 5039

The microquasar LS 5039 has recently been detected as a source of very high energy (VHE) $\gamma$-rays. This detection, that confirms the previously proposed association of LS 5039 with the EGRET source 3EG~J1824$-$1514, makes of LS 5039 a special system with observational data covering nearly all the electromagnetic spectrum. In order to reproduce the observed spectrum of LS 5039, from radio to VHE $\gamma$-rays, we have applied a cold matter dominated jet model that takes into account accretion variability, the jet magnetic field, particle acceleration, adiabatic and radiative losses, microscopic energy conservation in the jet, and pair creation and absorption due to the external photon fields, as well as the emission from the first generation of secondaries. The radiative processes taken into account are synchrotron, relativistic Bremsstrahlung and inverse Compton (IC). The model is based on a scenario that has been characterized with recent observational results, concerning the orbital parameters, the orbital variability at X-rays and the nature of the compact object. The computed spectral energy distribution (SED) shows a good agreement with the available observational data.

Gamma-ray emission from massive young stellar objects

Context.Massive stars form in dense and massive molecular cores. The exact formation mechanism is unclear, but it is possible that some massive stars are formed by processes similar to those that produce the low-mass stars, with accretion/ejection phenomena occurring at some point of the evolution of the protostar. This picture seems to be supported by the detection of a collimated stellar wind emanating from the massive protostar IRAS 16547-4247. A triple radio source is associated with the protostar: a compact core and two radio lobes. The emission of the southern lobe is clearly non-thermal. Such emission is interpreted as synchrotron radiation produced by relativistic electrons locally accelerated at the termination point of a thermal jet. Since the ambient medium is determined by the properties of the molecular cloud in which the whole system is embedded, we can expect high densities of particles and infrared photons. Because of the confirmed presence of relativistic electrons, inverse Compton and relativistic Bremsstrahlung interactions are unavoidable. Aims.We aim to make quantitative predictions of the spectral energy distribution of the non-thermal spots generated by massive young stellar objects, with emphasis on the particular case of IRAS 16547-4247. Methods.We study the high-energy emission generated by the relativistic electrons which produce the non-thermal radio source in IRAS 16547-4247. We also study the result of proton acceleration at the terminal shock of the thermal jet and make estimates of the secondary gamma rays and electron-positron pairs produced by pion decay. Results.We present spectral energy distributions for the southern lobe of IRAS 16547-4247, for a variety of conditions. We show that high-energy emission might be detectable from this object in the gamma-ray domain. The source may also be detectable in X-rays through long exposures with current X-ray instruments. Conclusions.Gamma-ray telescopes such as GLAST, and even ground-based Cherenkov arrays of new generation can be used to study non-thermal processes occurring during the formation of massive stars.

Extração de ferro de esmectita brasileira com emprego do método ditionito-citrato-bicarbonato

A natural clay from Campina Grande region (Paraíba, Brazil), with 8.57% of Fe2O3, was used to study the most appropriate condition to carry out the iron extraction, without altering the clay structure in a significant way. Samples were treated with the Dithionite-Citrate-Bicarbonate method (DCB) for 30 and 120 minutes (pH=9.1), and also with citric acid (pH=1.8; time=15min), at 75°C. Conductivity measurements, X-ray fluorescence, X-ray diffraction, energy-dispersive spectrometry, electron-diffraction with transmission electron microscopy and textural evaluation by nitrogen adsorption were done. The treatment in a basic medium was more selective for iron removal than in acid condition. The time of 30 minutes, with 1.6 g Na2S2O4/10 g clay, was the best condition for the iron extraction.