PLANETARY NEBULAE IN THE INNER MILKY WAY II: THE BULGE-DISK TRANSITION

In this work, a sample of planetary nebulae located in the inner-disk and bulge of the Galaxy is used in order to find the galactocentric distance which better separates these two populations, from the point of view of abundances. Statistical distance scales are used to study the distribution of abundances across the disk-bulge interface. A Kolmogorov-Smirnov test is used to find the distance at which the chemical properties of these regions better separate. The results of the statistical analysis indicate that, on the average, the inner population has lower abundances than the outer. Additionally, for the a-element abundances, the inner population does not follow the disk radial gradient towards the galactic center. Based on our results, we suggest a bulge-disk interface at 1.5 kpc, marking the transition between the bulge and inner-disk of the Galaxy as defined by the intermediate mass population.

SIMULATIONS OF WINDS OF WEAK-LINED T TAURI STARS. II. THE EFFECTS OF A TILTED MAGNETOSPHERE AND PLANETARY INTERACTIONS

Based on our previous work, we investigate here the effects on the wind and magnetospheric structures of weak-lined T Tauri stars due to a misalignment between the axis of rotation of the star and its magnetic dipole moment vector. In such a configuration, the system loses the axisymmetry presented in the aligned case, requiring a fully three-dimensional (3D) approach. We perform 3D numerical magnetohydrodynamic simulations of stellar winds and study the effects caused by different model parameters, namely the misalignment angle theta(t), the stellar period of rotation, the plasma-beta, and the heating index.. Our simulations take into account the interplay between the wind and the stellar magnetic field during the time evolution. The system reaches a periodic behavior with the same rotational period of the star. We show that the magnetic field lines present an oscillatory pattern. Furthermore, we obtain that by increasing theta(t), the wind velocity increases, especially in the case of strong magnetic field and relatively rapid stellar rotation. Our 3D, time-dependent wind models allow us to study the interaction of a magnetized wind with a magnetized extrasolar planet. Such interaction gives rise to reconnection, generating electrons that propagate along the planet`s magnetic field lines and produce electron cyclotron radiation at radio wavelengths. The power released in the interaction depends on the planet`s magnetic field intensity, its orbital radius, and on the stellar wind local characteristics. We find that a close-in Jupiter-like planet orbiting at 0.05 AU presents a radio power that is similar to 5 orders of magnitude larger than the one observed in Jupiter, which suggests that the stellar wind from a young star has the potential to generate strong planetary radio emission that could be detected in the near future with LOFAR. This radio power varies according to the phase of rotation of the star. For three selected simulations, we find a variation of the radio power of a factor 1.3-3.7, depending on theta(t). Moreover, we extend the investigation done in Vidotto et al. and analyze whether winds from misaligned stellar magnetospheres could cause a significant effect on planetary migration. Compared to the aligned case, we show that the timescale tau(w) for an appreciable radial motion of the planet is shorter for larger misalignment angles. While for the aligned case tau(w) similar or equal to 100 Myr, for a stellar magnetosphere tilted by theta(t) = 30 degrees, tau(w) ranges from similar to 40 to 70 Myr for a planet located at a radius of 0.05 AU. Further reduction on tau(w) might occur for even larger misalignment angles and/or different wind parameters.

PLANETARY NEBULAE IN THE INNER MILKY WAY: NEW ABUNDANCES

The study of planetary nebulae in the inner-disk and bulge gives important information on the chemical abundances of elements such as He, N, O, Ar, Ne, and on the evolution of these abundances, which is associated with the evolution of intermediate-mass stars and the chemical evolution of time Galaxy. We present accurate abundances of the elements He, N, 5, 0, Ar, and Ne for a sample of 54 planetary nebulae located towards the bulge of the Galaxy, for 33 of which the abundances are derived here for the first time. The abundances are obtained based on observations in the optical domain made at the National Laboratory for Astrophysics (LNA, Brazil). The data show a good agreement; with other results in the literature, in the sense that the distribution of the abundances is similar to that of those works.

PLANETARY NEBULAE AND THE CHEMICAL EVOLUTION OF THE MAGELLANIC CLOUDS

The determination of accurate chemical abundances of planetary nebulae (PN) in different galaxies allows us to obtain important constraints on chemical evolution models for these systems. We have a long-term program to derive abundances in the galaxies of the Local Group, particularly the Large and Small Magellanic Clouds. In this work, we present our new results on these objects and discuss their implications in view of recent abundance determinations in the literature. In particular, we obtain distance-independent correlations involving He, N, O, Ne, S, and Ar, and compare the results with data from our own Galaxy and other galaxies in the Local Group. As a result of our observational program, we have a large database of PN in the Galaxy and the Magellanic Clouds, so that we can obtain reliable constraints on the nucleosynthesis processes in the progenitor stars in galaxies of different metallicities.

Dynamic portrait of the planetary 2/1 mean-motion resonance - II. Systems with a more massive inner planet

This paper presents the second part in our study of the global structure of the planar phase space of the planetary three-body problem, when both planets lie in the vicinity of a 2/1 mean-motion resonance. While Paper I was devoted to cases where the outer planet is the more massive body, the present work is devoted to the cases where the more massive body is the inner planet. As before, outside the well-known Apsidal Corotation Resonances (ACR), the phase space shows a complex picture marked by the presence of several distinct regimes of resonant and non-resonant motion, crossed by families of periodic orbits and separated by chaotic zones. When the chosen values of the integrals of motion lead to symmetric ACR, the global dynamics are generally similar to the structure presented in Paper I. However, for asymmetric ACR the resonant phase space is strikingly different and shows a galore of distinct dynamical states. This structure is shown with the help of dynamical maps constructed on two different representative planes, one centred on the unstable symmetric ACR and the other on the stable asymmetric equilibrium solution. Although the study described in the work may be applied to any mass ratio, we present a detailed analysis for mass values similar to the Jupiter-Saturn case. Results give a global view of the different dynamical states available to resonant planets with these characteristics. Some of these dynamical paths could have marked the evolution of the giant planets of our Solar system, assuming they suffered a temporary capture in the 2/1 resonance during the latest stages of the formation of our Solar system.

An investigation of worn work roll materials used in the finishing stands of the hot strip mill for steel rolling

The surface failure characteristics of different work roll materials, i.e. High Speed Steel, High Chromium Iron and Indefinite Chill Iron, used in the finishing stands of a hot strip mill have been investigated using stereo microscopy, 3D optical profilometry, scanning electron microscopy and energy dispersive X-ray spectroscopy. The results show that the surface failure mechanisms of work rolls for hot rolling are very complex, involving plastic deformation, abrasive wear, adhesive wear, mechanical and thermal induced cracking, material transfer and oxidation. Despite the differences in chemical composition and microstructure, the tribological response of the different work roll materials was found to be strongly dependent on the material microstructure and especially the presence and distribution of microstructural constituents, such as the different carbide phases and graphite (in the case of Indefinite Chill Iron). Cracking and chipping of the work roll surfaces, both having a negative impact on work roll wear, are strongly influenced by the presence of carbides, carbide networks and graphite in the work roll surface. Consequently, the amount of carbide forming elements as well as the manufacturing process must be controlled in order to obtain an optimised microstructure and a predictable wear rate.

Caracterização do cDNA da NAD-MDH citosólica e da H+ ATPase Vacuolar no amadurecimento da anona (Annona cherimola Mill)

A Annona cherimola é um fruto exótico, com um sabor agradável. Este fruto tem um elevado potencial comercial, mas apresenta um tempo médio de vida curto devido ao seu rápido amadurecimento. Por esta razão é necessário conhecer melhor o processo de amadurecimento deste fruto. Na Região Autónoma da Madeira a cultura da anoneira é muito importante em termos comerciais. O processo de amadurecimento leva a diversas modificações bioquímicas e fisiológicas. Existem várias enzimas e substâncias que integram este processo. Neste trabalho iremos estudar os genes das enzimas malato desidrogenase e H+ ATPase vacuolar que estão envolvidos no processo de amadurecimento dos frutos. Utilizando as técnicas de RACE e sequenciação foi possível determinar a sequência nucleotídica do cDNA destes genes. O cDNA da malato desidrogenase é composto por 1364 nucleótidos, contendo uma zona 5’ UTR com 84 nucleótidos, uma zona 3’ UTR com 284 nucleótidos e um sinal de poliadenilação com a sequência AATAAA. A ORF apresenta 996 nucleótidos, codificando uma proteína com 332 aminoácidos. Para a H+ ATPase vacuolar foi amplificado o cDNA da subunidade C do domínio V1. Esta apresenta 799 nucleótidos, dos quais 36 são da 5’ UTR, 266 da 3’ UTR e 498 da ORF. A ORF codifica uma proteína com 166 aminoácidos.

Comparative analysis of the volatile fraction from Annona cherimola Mill. cultivars by solid-phase microextraction and gas chromatography–quadrupole mass spectrometry detection

The analysis of volatile compounds in Funchal, Madeira, Mateus and Perry Vidal cultivars of Annona cherimola Mill. (cherimoya) was carried out by headspace solid-phase microextraction (HS-SPME) combined with gas chromatography–quadrupole mass spectrometry detection (GC–qMSD). HS-SPME technique was optimized in terms of fibre selection, extraction time, extraction temperature and sample amount to reach the best extraction efficiency. The best result was obtained with 2 g of sample, using a divinylbenzene/carboxen/polydimethylsiloxane (DVB/CAR/PDMS) fibre for 30 min at 30 °C under constant magnetic stirring (800 rpm). After optimization of the extraction methodology, all the cherimoya samples were analysed with the best conditions that allowed to identify about 60 volatile compounds. The major compounds identified in the four cherimoya cultivars were methyl butanoate, butyl butanoate, 3-methylbutyl butanoate, 3-methylbutyl 3-methylbutanoate and 5-hydroxymethyl-2-furfural. These compounds represent 69.08 ± 5.22%, 56.56 ± 15.36%, 56.69 ± 9.28% and 71.82 ± 1.29% of the total volatiles for Funchal, Madeira, Mateus and Perry Vidal cultivars, respectively. This study showed that each cherimoya cultivars have 40 common compounds, corresponding to different chemical families, namely terpenes, esters, alcohols, fatty acids and carbonyl compounds and using PCA, the volatile composition in terms of average peak areas, provided a suitable tool to differentiate among the cherimoya cultivars.

Integrated valorization of Anona Cherimola Mill. seeds

Agricultural and agro-industrial residues are often considered both an environmental and an economical problem. Therefore, a paradigm shift is needed, assuming residues as biorefinery feedstocks. In this work cherimoya (Annona cherimola Mill.) seeds, which are lipid-rich (ca. 30%) and have a significant lignocellulosic fraction, were used as an example of a residue without any current valorization. Firstly, the lipid fraction was obtained by solvent extraction. Extraction yield varied from 13% to 28%, according to the extraction method and time, and solvent purity. This oil was converted into biodiesel (by base-catalyzed transesterification), yielding 76 g FAME/100 g oil. The obtained biodiesel is likely to be incorporated in the commercial chain, according to the EN14214 standard. The remaining lignocellulosic fraction was subjected to two alternative fractionation processes for the selective recovery of hemicellulose, aiming different products. Empirical mathematical models were developed for both processes, aiming future scale-up. Autohydrolysis rendered essentially oligosaccharides (10 gL-1) with properties indicating potential food/feed/pharmacological applications. The remaining solid was enzymatically saccharified, reaching a saccharification yield of 83%. The hydrolyzate obtained by dilute acid hydrolysis contained mostly monosaccharides, mainly xylose (26 gL-1), glucose (10 gL-1) and arabinose (3 gL-1), and had low content of microbial growth inhibitors. This hydrolyzate has proven to be appropriate to be used as culture media for exopolisaccharide production, using bacteria or microbial consortia. The maximum conversion of monosaccharides into xanthan gum was 0.87 g/g and kefiran maximum productivity was 0.07 g.(Lh)-1. This work shows the technical feasibility of using cherimoya seeds, and materials as such, as potential feedstocks, opening new perspectives for upgrading them in the biorefinery framework.

Novo sistema hidropónico aplicado à produção do tomate cereja (Lycopersicum esculentum Mill. var Moscatel RZ)

A hidroponia é uma técnica poderosa na utilização eficiente dos recursos agrícolas, pois permite um ganho quer na produtividade, quer na qualidade do fruto. Atualmente os sistemas hidropónicos utilizados em plantas de médio porte não são os mais adequados, sendo esta uma área a explorar. Neste trabalho criou-se um novo sistema hidropónico (Deep Large Flow Technique- DLFT) para aplicação a plantas de médio porte e avaliou-se o seu impacto no crescimento, produtividade, biomassa e qualidade do tomate cereja (Solanum lycopersicum var. Moscatel RZ). O sistema de cultivo tradicional (solo) e semi-hidropónico (suporte com fibra de coco) serviram como base de comparação. Observou-se que após 31 dias as plantas cultivadas no novo sistema hidropónico obtiveram um crescimento acentuado, apresentando 3x mais frutos. Em termos de produtividade, os sistemas hidropónicos foram iguais, sendo o sistema tradicional 4x inferior. O total de biomassa foi significativamente maior no novo sistema hidropónico, com mais 20% e 88% que o sistema semi-hidropónico e tradicional, respetivamente. As plantas produzidas no sistema DLFT apresentaram frutos com qualidade superior, com um rácio de monossacarídeos/acidez de 6,6 mg/g. O conteúdo total de ácidos gordos nos frutos cultivados com este sistema foi 39% e 44% superior aos do semihidropónico e do tradicional. Contrariamente, o conteúdo de flavonóides foi inferior nos frutos cultivados com o novo sistema hidropónico, tendo os frutos do sistema tradicional e do sistema semi-hidropónico 40% e 10% maior teor desta família de compostos. Os resultados obtidos neste estudo demonstram que a utilização do novo sistema hidropónico na produção de plantas de médio porte, aumenta o crescimento, a acumulação de biomassa e a qualidade do fruto. Assim, permite ao produtor reduzir os custos, rentabilizar a produção (menor tempo de produção), valorizar a biomassa da planta e aumentar a qualidade do produto. Também, através dos teores de carotenóides, ácidos gordos e polifenóis poderá inferir-se que ocorreu um menor impato dos stressses abióticos subjacentes aos sistemas nas plantas produzidas pelo sistema DLFT.

Sinterização de aço inoxidável reforçado com partículas nanométricas dispersas de carbeto de nióbio - NbC

Metal powder sintering appears to be promising option to achieve new physical and mechanical properties combining raw material with new processing improvements. It interest over many years and continue to gain wide industrial application. Stainless steel is a widely accepted material because high corrosion resistance. However stainless steels have poor sinterability and poor wear resistance due to their low hardness. Metal matrix composite (MMC) combining soft metallic matrix reinforced with carbides or oxides has attracted considerable attention for researchers to improve density and hardness in the bulk material. This thesis focuses on processing 316L stainless steel by addition of 3% wt niobium carbide to control grain growth and improve densification and hardness. The starting powder were water atomized stainless steel manufactured for Höganäs (D 50 = 95.0 μm) and NbC produced in the UFRN and supplied by Aesar Alpha Johnson Matthey Company with medium crystallite size 16.39 nm and 80.35 nm respectively. Samples with addition up to 3% of each NbC were mixed and mechanically milled by 3 routes. The route1 (R1) milled in planetary by 2 hours. The routes 2 (R2) and 3 (R3) milled in a conventional mill by 24 and 48 hours. Each milled samples and pure sample were cold compacted uniaxially in a cylindrical steel die (Ø 5 .0 mm) at 700 MPa, carried out in a vacuum furnace, heated at 1290°C, heating rate 20°C stand by 30 and 60 minutes. The samples containing NbC present higher densities and hardness than those without reinforcement. The results show that nanosized NbC particles precipitate on grain boundary. Thus, promote densification eliminating pores, control grain growth and increase the hardness values

Estudo sobre a redução aluminotérmica de Ta2O5 e TiO2 usando descarga de cátodo oco

In this study it was used two metallic oxides, Ta2O5 and TiO2, in order to obtain metallic powders of Ta and Ti through aluminothermic reduction ignited by plasma. Ta2O5 and TiO2 powders were mixed with Al in a planetary mill, using different milling times. A thermal analysis study (DTA and TG) was carried out, in order to know the temperature to react both the mixtures. Then, these mixtures were submitted to a hollow cathode discharge, where they were reacted using aluminothermic reduction ignited by plasma. The product obtained was characterized by XRD and SEM, where it was proven the possibility of producing these metallic particles, different from the conventional process, where metallic ingots are obtained. It was verified that the aluminothermic reduction ignited by plasma is able to produce metallic powders of Ta and Ti, and a higher efficiency was observed to the process with Ta2O5-Al mixtures. Among different microstructural aspects observed, it can be noted the presence of metallic nanoparticles trapped into an Al2O3 matrix, besides acicular structures (titanium) and dendritic structures (tantalum), which are a product characteristic from a fast cooling

Estimativa da área foliar de plantas daninhas: Solanum americanum Mill

A maria pretinha (Solanum americanum Mill) é uma planta daninha infestante de diversas culturas e além da competição pode causar outros problemas. Nos estudos envolvendo a biologia e o controle de plantas daninhas, a área foliar é uma das mais importantes características a serem avaliadas, mas tem sido pouco estudada porque sua determinação exige equipamentos sofisticados ou utiliza técnicas destrutivas. Visando obter equações que permitissem a estimativa da área foliar desta planta daninha utilizando características lineares do limbo foliar, facilmente mensuráveis em plantas no campo, foram estudadas correlações entre a área foliar real e as seguintes características das folhas: comprimento ao longo da nervura principal (C), largura máxima do limbo (L) e o produto (C x L). Para tanto, foram mensuradas 200 folhas coletadas de plantas sujeitas às mais diversas condições ecológicas em que a espécie sobrevive, considerando-se todas as folhas das plantas desde que não apresentassem deformações oriundas de fatores, tais como, pragas, moléstias e granizo. Todas as equações, lineares simples, geométricas e exponenciais, permitiram boa estimativa da área foliar (Af) da maria pretinha. do ponto de vista prático, sugere-se optar pela equação linear simples envolvendo o produto (C x L), a qual apresentou o menor QM Resíduo. Assim, a estimativa da área foliar de S. americanum pode ser efetuada pela equação AF = 0,5632 x (C x L), com coeficiente de determinação (R2) de valor igual a 0,9516.

Nutrição mineral de hortaliças XXVII: tolerância de cultivares de tomateiro (Lycopersicon esculentum Mill) ao alumínio e ao manganês

Dois experimentos foram conduzidas, em condições de casa-de--vegetação com o objetivo de caracterizar diferenças entre cultivares de tomateiro (Lycopersvcum esculentum Mill) com relação à tolerância ao alumínio e ao manganês. No primeiro experimento foram cultivados em Latossol Roxo (solo ácido, com níveis elevados de alumínio e manganês), seis cultivares de tomateiro: Santa Cruz Kada, Angela IAC 3946, Vital, Roma VF, Pavebo 220 e Ronita N, os três primeiros de crescimento indeterminado e os restantes de crescimento determinado. No segundo experimento, os cultivares Santa Cruz Kada e Ronita N que apresentaram um contraste de desenvolvimento no solo ácido, foram cultivados em solução nutritiva de HOAGLAND & ARNON, modificada para níveis de manganês (0,5 ; 1,5 e 3,0 ppm) e com adição de níveis de alumínio (0,0; 10,0 e 20,00 ppm). Os resultados obtidos permitiram indicar o cultivar Santa Cruz Kada como mais tolerante ao alumínio que o cultuar Ronita N. A maior sensibilidade ao alumínio do cultivar Ronita N foi associada com uma maior exigência em cálcio e fósforo, com uma maior absorção de alumínio e também com efeito depressivo do alumínio na absorção dos nutrientes mencionados, em relação ao cultivar Santa Cruz Kada. A tolerância do cultivar Santa Cruz Kada ao alumínio apesar de ser maior que a do Ronita N pode ser considerada de grau relativamente baixo, podendo-se esperar ainda, boas respostas dessas plantas à calagem nos cultivares em solos ácidos. O comportamento dos cultivares frente aos níveis de manganês em solução nutritiva foi semelhante, não sendo observado qualquer efeito prejudicial do elemento nos níveis empregados.

Sazonalidade dos ductos secretores e óleo essencial de Foeniculum vulgare var. vulgare Mill. (Apiaceae)

Este trabalho teve como objetivo analisar os ductos secretores e o óleo essencial das folhas de Foeniculum vulgare em diferentes épocas do ano. Para esta finalidade, foram realizados estudos de caracterização anatômica, bem como anatomia comparada dos ductos secretores e testes histoquímicos das folhas. O óleo essencial foi obtido de folhas e frutos, por hidrodestilação em aparelho de Clevenger e analisados quantitativamente e qualitativamente por cromatografia em fase gasosa acoplada ao espectrômetro de massa, realizando-se análises seguidas de três réplicas para folhas coletadas durante o inverno e primavera, e frutos no verão. Os resultados encontrados para os ductos secretores de óleo corresponderam à redução do teor de óleo essencial nas folhas coletadas no final da primavera. O componente majoritário do óleo essencial de folhas e frutos foi o trans-anetol, durante todas as estações do ano. Portanto, evidenciou-se que os ductos secretores e teor de óleo essencial estão relacionados, bem como os constituintes químicos também estão sujeitos a sazonalidade, conforme o estágio fenológico da planta.