Interação estrela planeta: sobre o magnetismo de planetas gigantes gasosos

In this thesis we analyze the effects that the presence of a near gas giant planet can cause in its host star. It has been argued that the star planet interaction can cause changes in the coronal and chromospheric stellar activity. With this in mind, we analyze a sample of 53 extrasolar planets orbiting F, G and K main sequence stars, among them three super-Earths. In this analysis, we look for evidence of changes in the chromospheric activity due to the proximity of the giant planet. We show that, so far, there is not enough evidence to support such a hypothesis. Making use of the same sample and also taking in account available data for the Solar System, we revisit the so-called magnetic Bode s law. This law proposes the existence of a direct relationship between magnetism and rotation. By using estimations for the stellar and planetary magnetic momentM and the angular momentumL, we construct a Blackett s diagram (logL 􀀀logM). In this diagram is evident that the magnetic Bode s law is valid for both the Solar System and the new planetary systems

Atividade cromosférica induzida por planetas extrasolares gigantes

In the present work, we have analyzed the behavior of the chromospheric activity of stars with planets, as a function of different planetary parameters, searching for possible effects of planets on the chromosphere of the hosting star. For this study we have selected a sample of 73 main sequence stars with planets, of spectral types F, G and K. Our analysis shows that among stars with planets presenting semi-major axis smaller than 0.15 AU, a few ones present enhanced CaII emission flux, paralleling recent results found in the literature for coronal X-ray flux. Nevertheless, in contrast to Kashyap et al. (2008), who claim that enhanced X-ray flux in stars with planets is associated to massive close-in planetary companions, we suggest that such an aspect, at least in the context of CaII emission flux, is rather an effect of stellar sample selection. We have also studied the behavior of the CaII emission as a function of orbital parameters such as orbital period and eccentricity, and no clear trend was found, reinforcing our present suggestion that enhanced chromospheric activity in stars with planets is an intrinsic stellar phenomenon

Um estudo da abundância de lítio, rotação, atividade cromosférica e magnetismo das estrelas análogas e gêmeas solares

The study physical process that control the stellar evolution is strength influenced by several stellar parameters, like as rotational velocity, convective envelope mass deepening, and magnetic field intensity. In this study we analyzed the interconnection of some stellar parameters, as Lithium abundance A(Li), chromospheric activity and magnetic field intensity as well as the variation of these parameters as a function of age, rotational velocity, and the convective envelope mass deepening for a selected sample of solar analogs and twins stars. In particular, we analyzed the convective envelope mass deepening and the dispersion of lithium abundance for these stars. We also studied the evolution of rotation in subgiants stars, because its belong to the following evolutionary stage of solar analogs, and twins stars. For this analyze, we compute evolutionary models with the TGEC code to derive the evolutionary stage, as well as the convective envelope mass deepening, and derive more precisely the stellar mass, and age for this 118 stars. Our Investigation shows a considerable dispersion of lithium abundance for the solar analogs stars. We also realize that this dispersion is not by the convective zone deep, in this way we observed which the scattering of A(Li) can not be explained by classical theories of mixing in the convective zone. In conclusion we have that are necessary extra-mixing process to explain this decrease of Lithium abundance in solar analogs and twins stars. We analyzed the subgiant stars because this are the subsequent evolutionary stage after the solar analogs and twins stars. For this analysis, we compute the rotational period for 30 subgiants stars observed by Co- RoT satellite. For this task we apply two different methods: Lomb-Scargle algorithm, and the Plavchan Periodogram. We apply the TGEC code we compute models with internal distribution of angular momentum to confront the predict results with the models, and the observational results. With this analyze, we showed which solid body rotation models are incompatible with the physical interpretation of observational results. As a result of our study we still concluded that the magnetic field, convective envelope mass deepening, and internal redistribution of angular momentum are essential to explain the evolution of low-mass stars, and its observational characteristics. Based on population synthesis simulation, we concluded that the solar neighborhood presents a considerable quantity of solar twins when compared with the discovered set nowadays. Altogether we foresee the existence around 400 solar analogs in the solar neighborhood (distance of 100 pc). We also study the angular momentum of solar analogs and twins, in this study we concluded that added angular momentum from a Jupiter type planet, putted in the Jupiter position, is not enough to explain the angular momentum predicted by Kraft law (Kraft 1970)

Evolução da atividade cromosférica, abundância de lítio e rotação das estrelas análogas e gêmeas solares

The study of solar-type stars also includes the familiar solar analogs and twins. These objects have been one of the major research subjects in astrophysics nowadays. A direct comparison of solar activity with chromospheric activity indices for a set of stars very similar to the Sun (twins and analogs) provides an excellent opportunity to study the evolution of stellar activity on timescales of the order of the lifetime on the main sequence. This work deals with the relationship between the abundance of lithium, chromospheric activity, X-ray emission and rotation period in terms of stellar ages. We explore the influence of stellar evolution in the global properties of the stars and the aspects linked to its coronal, chromospheric and magnetic activity. Our main objective is to probe the law of decay of each of these parameters based on a sample of stars classified as well-connected as analogs stars and solar twins.

Um estudo sobre a interação estrela-planeta a partir da relação massa-período planetário com a atividade estelar

n this work, we analyze the behavior of the chromospheric and coronal activities as a function of the mass and the orbital period of extrasolar planets which were detected by transit technique. So we look for possible effects of the planet on the star s chromosphere and corona. For this study we selected a sample of 48 stars with chromospheric activity indicator and 23 with coronal activity indicator. Our work is based on the work from Pont et al. (2011) in order to study stars with planets which were obtained by transit technique. Furthermore, we studied the relationship between planetary mass and orbital period with the chromospheric and coronal activity in order to better understand which influences the planets cause in the outer layers of stellar atmosphere. In our analysis we can observe that the mass of the planets exerts no influence in the stellar activity. However, we observed that the stellar coronal and chromospheric activities decrease with the increase of the orbital period of the planet

Um estudo sobre a interação estrela-planeta a partirda relação massa-período planetário com a atividade estelar

In this work, we analyze the behavior of the chromospheric and coronal activities as a function of the mass and the orbital period of extrasolar planets which were detected by transit technique. So we look for possible effects of the planet on the star s chromosphere and corona. For this study we selected a sample of 48 stars with chromospheric activity indicator and 23 with coronal activity indicator. Our work is based on the work from Pont et al. (2011) in order to study stars with planets which were obtained by transit technique. Furthermore, we studied the relationship between planetary mass and orbital period with the chromospheric and coronal activity in order to better understand which influences the planets cause in the outer layers of stellar atmosphere. In our analysis we can observe that the mass of the planets exerts no influence in the stellar activity. However, we observed that the stellar coronal and chromospheric activities decrease with the increase of the orbital period of the planet

Processos de aquecimento na alta atmosfera estelar: emissão coronal em raio-x e emissão cromosférica em CaII

In the present work we study the processes of heating in the high stellar atmosphere, with base in an analysis of behavior of the cromospheric and coronal emission for a sample of single stars classified as giant in the literature. The evolutionary status of the stars of the sample was determined from HIPPARCOS satellite trigonometric parallax measurements and from the Toulouse Genéve code. In this study we show the form of behavior of the CaII emission flux in spectral lines H and K F(CaII) and the X-ray emission flux in function of the rotation, number of Rossby Ro and depth in mass of the convective envelope. In this analysis we show that while the cromospheric activity is dominated clearly by a physical process of heating associated with the rotation, like a magnetic field produced by dynamo effect, the coronal activity seems to be influenced for a mechanism independent of the rotation. We show also that the effective role of the depth in massa of the convective envelope on the stellar activity has an important effect in the responsible physical process for the behavior of the activity in the atmosphere of the stars.

Sobre a relação entre rotação, atividade crosmosférica e abundância de lítio em estrelas subgigantes

The connection between rotation, CaII emission flux and lithium abundance is analyzed for a sample of subgiant stars, with evolutionary status was determined from the Toulouse-Geneve code and HlPPARCOS trigonometric parallax measurements. We noted that the distribution of rotation and CaII emission flux, as a function of effective temperature, shows a discontinuity located around the same spectral type, F8IV. Stars located blueward of this spectral type, exhibit a large spread of values of rotation and CaII flux, whereas stars redward of F8lV show essentially low ratation anel low CaII flux. The strength of these declines nevertheless, depends on stellar mass. The distribution of lithium abundances also shows a discontinuity, however with behavior a little more complex for subgiants with mass lower than about 1.2 Solar Masses, this decrease is observed later than that in rotation and CaII flux, whereas for masses higher than 1.2 Solar Masses the decrease in lithium abundance is located around the spectral type F8IV. The discrepancy between the location of the discontinuities of rotation and CaII flux and log n(Li) for stars with masses lower than 102 Solar Masses, seems to reflect the sensitivity of these phenomena to the mass of the convective envelope. The drop in rotation, which results mostly from a magnetic braking, requires an increase in the mass of the convective envelope less than that required for the decrease in lithium abundance The location of the discontinuity in log n( Li) in the same region of the discontinuity ties in rotation and CaII flux, for stars with masses higher than 1.2 Solar Masses, may also be explained by the behavior of the deepening of the convective envelope. In contrast to the relationship between rotation and CaII flux the relationship between lithium abundance and rotation shows no dear tendency toward linear behavior. Similarly, the same tendency is observed in the relationship between lithium abundance and CaII flux in spite of these facts, subgiants with high lithium content also have high rotation and high CaII emission flux. We also observed that stars with high lithium content present, in its majority, an undeveloped convective envelope, whereas stars with low lithium content have a developed convective envelope. In the case of the rotation, stars with undeveloped convective envelope, show rotational velocities as much high as low, whereas stars with developed convective envelope only present low rotation

O índice BODE reflete o nível de atividade física na vida diária de pacientes com DPOC?

Objectives: To study the relationship between the level of physical activity in daily life and disease severity assessed by the BODE index in patients with chronic obstructive pulmonary disease (COPD). Methods: Sixty-seven patients with COPD (36 men) with forced expiratory volume in the first second (FEV(1)) of 39 (27-47)% predicted and age of 66 (61-72) years old were evaluated by spirometry, dyspnea levels (measured by the Medical Research Council scale, MRC) and by the 6-minute walking test (6MWT). The BODE index was calculated based on the body mass index (weight/height(2)), FEV(1), MRC and 6MWT, and then the patients were divided in four quartiles according to their scores (Quartile I: 0 to 2 points, n=15; Quartile II: 3 to 4 points, n=20; Quartile III: 5 to 6 points, n=23; Quartile IV: 7 to 10 points, n=9). Two activity monitors (DynaPort (R) and SenseWear (R)) were used to evaluate the level of physical activity in daily life. The Kruskal-Wallis test (Dunns's post-hoc test), the Mann-Whitney test and the Spearman Correlation Coefficient were used for statistical analysis. Results: There were modest correlation between the BODE index and the time spent walking per day, the total daily energy expenditure and the time spent in moderate and vigorous activities per day (-0.32 <= r <=- 0.47; p <= 0.01 for all variables). When comparing the pooled quartiles I+II with III+IV, there were significant difference between the time spent walking per day, the total daily energy expenditure and the time spent in moderate activities per day (p <= 0.05). Conclusion: The level of physical activity in daily life has a modest correlation with the classification of COPD severity assessed by the BODE index, reflecting only differences between patients with classified as mild-moderate and severe-very severe COPD.

Propriedades físicas de planetas extrasolares

ROTATION is one the most important aspects to be observed in stellar astrophysics. Here we investigate that particularly in stars with planets. This physical parameter supplies information about the distribution of angular momentum in the planetary system, as well as its role on the control of dierent phenomena, including coronal and cromospherical emission and on the ones due of tidal effects. In spite of the continuous solid advances made on the study of the characteristics and properties of planet host stars, the main features of their rotational behavior is are not well established yet. In this context, the present work brings an unprecedented study about the rotation and angular momentum of planet-harbouring stars, as well as the correlation between rotation and stellar and planetary physical properties. Our analysis is based on a sample of 232 extrasolar planets, orbiting 196 stars of dierent luminosity classes and spectral types. In addition to the study of their rotational behavior, the behavior of the physical properties of stars and their orbiting planets was also analyzed, including stellar mass and metallicity, as well as the planetary orbital parameters. As main results we can underline that the rotation of stars with planets present two clear features: stars with Tef lower than about 6000 K have slower rotations, while among stars with Tef > 6000 K we and moderate and fast rotations, though there are a few exceptions. We also show that stars with planets follow mostly the Krafts law, namely < J > / v rot. In this same idea we show that the rotation versus age relation of stars with planets follows, at least qualitatively, the Skumanich and Pace & Pasquini laws. The relation rotation versus orbital period also points for a very interesting result, with planet-harbouring stars with shorter orbital periods present rather enhanced rotation

A atividade policial em face da Lei de combate ao crime organizado / Ivan Lira de Carvalho. --

Palestra proferida em 17.05.96, em comemoração ao aniversário de criação do Sindicato dos Servidores da Polícia Federal no Rio Grande do Norte.

Resolu????o simplificadora de formalidades e procedimentos relativos aos atos de que trata o art. 54 da Lei n?? 8.884 de 11 de junho 1994

O controle de ag??ncias de defesa da concorr??ncia sobre a estrutura dos mercados constitui pr??tica comum em pa??ses maduros e vem ganhando import??ncia crescente em economias emergentes. Tal atividade envolve exame de atos de concentra????o econ??mica tais como fus??es, aquisi????es, joint ventures ou incorpora????es. No Brasil este tipo de controle ?? recente, tendo sido institu??do pela Lei n?? 8.884, de junho de 1994. Desde ent??o, o Conselho Administrativo de Defesa da Concorr??ncia - CADE julgou 29 (vinte e nove) atos de concentra????o, em contraste com a experi??ncia secular de pa??ses como EUA, Canad?? e Austr??lia e de v??rias d??cadas nas na????es europ??ias depois da Segunda Guerra. A exemplo de v??rias outras ??reas de pol??tica p??blica, tornou-se imperativo agilizar os ??rg??os de defesa da concorr??ncia. Isto decorre, entre outros fatores, do intenso processo de reestrutura????o produtiva em curso no pa??s associados ?? desestatiza????o e abertura da economia. Diante das circunst??ncias descritas, ?? preciso assegurar agilidade, transpar??ncia, excel??ncia t??cnica no processo decis??rio e estabilidade de regras, todos ingredientes indispens??veis para gerar seguran??a jur??dica. Esta ??ltima, por seu turno, diminui o risco do investimento, estimulando invers??es, produ????o e emprego. Nesse sentido, o CADE promoveu mudan??as importantes no procedimento de an??lise de atos de concentra????o em colabora????o com a Secretaria de Direito Econ??mico do Minist??rio da Justi??a (SDE) e a Secretaria de Acompanhamento Econ??mico do Minist??rio da Fazenda (SEAE) mediante a edi????o da Resolu????o 5, de 28 de agosto de 1996

O parlamento e a regulação das comunicações : estudo sobre a atividade legislativa do congresso nacional para a radiodifusão

Dissertação (mestrado)—Universidade de Brasília, Faculdade de Comunicação, Programa de Pós-Graduação em Comunicação, 2016.

Estudo físico-químico comparativo de sistemas nanoestruturados contendo indometacina ou seu éster etílico e avaliação in vivo da atividade antiedematogênica

Nanocápsulas (NC), nanoesferas (NS) e nanoemulsão (NE) são propostas na literatura como carreadores submicrométricos de fármacos. Os objetivos deste trabalho são realizar um estudo comparativo para diferenciar o comportamento cinético desses sistemas e avaliar a influência da espessura da parede polimérica das NC no perfil de liberação de um modelo lipofílico de fármaco a partir de diversas formulações preparadas com diferentes concentrações de poli(-caprolactona) (PCL). Com esse propósito, o éster etílico de indometacina (IndOEt) foi associado a cada sistema e a sua hidrólise alcalina foi realizada para simular uma condição sink. As suspensões aquosas foram tratadas com solução aquosa de NaOH e a modelagem matemática dos perfis de consumo do IndOEt foi realizada. Uma vez que os derivados éster de indometacina têm sido relatados como inibidores seletivos da ciclooxigenase-2, também constitui objetivo deste trabalho avaliar a atividade antiedematogênica em ratos do IndOEt associado aos nanocarreadores através da inibição do edema em pata de rato induzido por carragenina. O IndOEt apresentou consumo total em 24 horas para NC, 12 horas para NS e 8 horas para NE. A modelagem matemática demonstrou que os perfis cinéticos apresentaram uma fase de liberação rápida, com tempo de meia-vida de 5,9, 4,4 e 2,7 minutos, e uma fase de liberação sustentada com tempos de meia-vida de 288,8, 87,7 e 147,5 minutos, respectivamente. Comparando-se os resultados, as NC apresentaram os maiores tempos de meia-vida para o modelo lipofílico de fármaco associado aos nanocarreadores Para todas as formulações preparadas com diferentes concentrações de PCL, a modelagem matemática dos perfis demonstrou que quanto menor a concentração de polímero empregada, mais rápido é o consumo do éster. Para todos os sistemas estudados, um ajuste satisfatório dos dados experimentais ao modelo da Lei das Potências foi obtido. A incorporação do IndOEt em NC e NS apresentou atividade antiedematogênica após a administração oral das formulações. Por outro lado, a associação do IndOEt na NE não inibiu o edema induzido pela carragenina.

Regendo a atividade regulatória: a nova legislação das agências reguladoras federais no Brasil

Os processos e as instituições regulatórias são assuntos prioritários da agenda governamental, por tratarem-se de assunto dinâmico que envolve uma mudança na cultura administrativa do país. Um dos grandes desafios das agências reguladoras brasileiras tem sido desempenhar suas funções de forma autônoma e imparcial com o objetivo de promover confiança e transparência ao mercado e à sociedade. Este estudo buscou realizar uma análise do conteúdo e das repercussões das mudanças ora em curso no Brasil, em especial daquelas contidas na proposta enviada pelo governo federal brasileiro ao Congresso Nacional dispondo sobre a nova Lei Geral das Agências reguladoras (Projeto de Lei 3337/2004), com o fito de promover mudanças no modelo de organização institucional e funcionamento desses entes regulatórios. Com esse fim, de início, foram descritos os fundamentos teóricos da regulação, com a apresentação do processo de criação das agências reguladoras federais brasileiras e suas características determinantes. Após a fundamentação, foram detalhados os pontos principais do Projeto de Lei 3337/2004, e seu substitutivo, elaborado pelo Deputado Leonardo Picciani. O próximo capítulo, Governança Regulatória, apresentou as políticas de reforma regulatória, seus desafios no Brasil, e delineou o Programa de Fortalecimento da Capacidade Institucional para Gestão em Regulação (PRO-REG). O estudo deu prosseguimento à análise por meio da apresentação das boas práticas à qualidade regulatória, enfatizando a importância da participação social no processo regulatório, e também da abordagem da experiência internacional. Item complementar para a compreensão e visão geral do estudo, a supervisão regulatória foi também conceituada e justificada, seguida pela abordagem da criação da Unidade de Supervisão Central e da experiência internacional. Por último, em análise final do tema, apoiada por grande pesquisa bibliográfica e documental, e por entrevistas concedidas pelos ocupantes dos dois maiores cargos da Superintendência de Abastecimento da Agência Nacional do Petróleo, Gás Natural e Biocombustíveis, procurou-se mostrar a imprescindibilidade do desenvolvimento e implementação de uma estratégia de qualidade regulatória que permita uma abordagem consistente.