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

Parâmetros físico-químicos de estrelas com planetas na missão CoRoT

In the present study we compute the atmospheric parameters (Teff , log g and vmic, [Fe/H]) and chemical abundance of 16 ions (Fe I, Fe II, O I, Si I, Na I, Mg I, Al I, Ca I, Ti I, Co I, Ni I, Rb I, Zr I, Ba II, La II and Cr I) for 16 solar-like stars with masses between 0:8 and 1:2 Mfi aproximatedly, including 10 planet-host stars detected by the CoRoT Space Mission. For this study, we use data from the ESO public archive: (i) high resolution spectra (R 47000) from the UVES spectrograph on the VLT/UT2-ESO (for 7 stars, covering the wavelength range 3450-4515 Å and 5500-9400 Å) and (ii) high resolution spectra from HARPS spectrograph on the La Silla-ESO 3.60 m telescope (for 9 stars, covering the wavelength range 4200-6865 Å). Our spectral analysis is based on MARCS models of atmosphere and Turbospectrum spectroscopic tools. On the base of the computed parameters, the referred abundances appears to follow the same behavior of the solar curve abundances. Further, one observes a signifficant correlation between the abundance ratio [m/Fe] and condensation temperature (Tc) of refractory elements (Tc > 900 K). The behavior of the projected rotational velocity (v sin i) versus the computed abundances [m/Fe] is also analyzed, presenting no clear trends. This study oers additional constraints to trace the evolutive history of solar-like stars with planets, including the search for chemical dierences between stars with and without transit planets and anomalies in the studied abundances

Sobre a composição química em estrelas evoluídas do aglomerado aberto M67

The Galaxy open clusters have a wide variety of physical properties that make them valuable laboratories for studies of stellar and chemical evolution of the Galaxy. In order to better settle these properties we investigate the abundances of a large number of chemical elements in a sample of 27 evolved stars of the open cluster M67 with different evolutionary stages (turn-off, subgiant and giant stars). For such a study we used high-resolution spectra (R 47 000) and high S/N obtained with UVES+FLAMES at VLT/UT2, covering the wavelength interval 4200-10 600 Å. Our spectral analysis is based on the MARCS models of atmosphere and Turbospectrum spectroscopic tool. The oxygen abundances were determined from the [O I] line at 6300 Å. In addition, we have also computed abundances of Si I, Na I, Mg I, Al I, Ca I, Ti I, Co I, Ni I, Zr I, La II and Cr I. The abundances investigated in this work, combined with their stellar parameters, offers an opportunity to determine the level of mixing and convective dilution of evolved stars in M67. Based on the obtained parameters, the abundances of these seem to follow a similar trend to the curve of solar abundances. Additionally, following strategies of other studies have investigated the relative abundances as a function of effective temperature and metallicity, where it was possible to observe an abundance of Na, Al and Si to the stars in the field of giants. A large dispersion from star to star, is observed in the ratios [X / Fe] for the Co, Zr and La, and the absence of Zr and La, in the stars of the turn-off. Comparisons made between our results and other studies in the literature show that values of abundances are in agreement and close to the limits of the errors

Sistemas binários eclipsantes na missão CoRot

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior

Dysglycemias in pregnancy: from diagnosis to treatment. Brazilian consensus statement

There is an urgent need to find consensus on screening, diagnosing and treating all degrees of DYSGLYCEMIA that may occur during pregnancies in Brazil, considering that many cases of DYSGLYCEMIA in pregnant women are currently not diagnosed, leading to maternal and fetal complications. For this reason the Brazilian Diabetes Society (SBD) and the Brazilian Federation of Gynecology and Obstetrics Societies (FEBRASGO), got together to introduce this proposal. We present here a joint consensus regarding the standardization of clinical management for pregnant women with any degree of Dysglycemia, on the basis of current information, to improve medical assistance and to avoid related complications of Dysglycemia in pregnancy to the mother and the fetus. This consensus aims to standardize the diagnosis among general practitioners, endocrinologists and obstetricians allowing the dissemination of information in basic health units, public and private services, that are responsible for screening, diagnosing and treating disglycemic pregnant patients.

Cirurgia não ginecológica em pacientes com câncer de ovário

OBJETIVO: avaliar a freqüência da utilização de procedimentos cirúrgicos não ginecológicos no tratamento do câncer de ovário, assim como descrever as suas complicações. MÉTODOS: foram incluídas retrospectivamente 82 pacientes, atendidas no período de fevereiro de 1999 a outubro de 2003, e que haviam sido submetidas a laparotomia para tratamento cirúrgico do câncer de ovário. Foram incluídas no estudo apenas pacientes com adenocarcinoma epitelial de ovário. A média de idade foi de 54,1±15,1 anos, variando de 22 a 89 anos. O estadiamento (FIGO) mostrou 5 pacientes no estádio I (6,1%), 18 pacientes no II (21,9%), 40 pacientes no III (48,8%) e 19 pacientes no IV (23,2%). As pacientes foram divididas em 2 grupos: aquelas em que foram realizados exclusivamente procedimentos ginecológicos e aquelas com realização de procedimentos não ginecológicos. As diferenças entre as médias foram analisadas pelo teste t de Student. As comparações entre grupos independentes foram feitas pelo teste do chi2. RESULTADOS: em 35 pacientes (42,7%) foram realizados procedimentos cirúrgicos não ginecológicos, incluindo: 17 colostomias, 16 enterectomias, oito peritonectomias pélvicas, sete colectomias, cinco ressecções parciais de cúpula frênica, quatro cistectomias parciais, quatro esplenectomias, duas ileostomias e uma hepatectomia parcial. Todas as pacientes submetidas a procedimentos não ginecológicos apresentavam-se nos estádios III e IV. Esse grupo apresentou maior tempo cirúrgico (5,3±1,4 versus 3,1±0,9 horas); p<0,001). Os grupos não mostraram diferenças significativas em relação à necessidade de hemotransfusão (42,2 versus 40%; p=0,512) e tempo de internação (11,5±7,2 versus 10±9,9 dias; p=0,454). A realização de procedimentos cirúrgicos não ginecológicos associou-se a maior taxa de complicações pós-operatórias 37% versus (17,1%; p=0,042), sendo que duas pacientes desse grupo (2,4%) evoluíram para o óbito. CONCLUSÕES: os procedimentos cirúrgicos não ginecológicos são freqüentemente empregados no tratamento de pacientes com câncer de ovário. A realização dessas cirurgias está associada a maior tempo cirúrgico e maior taxa de complicações pós-operatórias.

Valor nutritivo da raiz e folhas da mandioca para a tilápia do nilo

The aim was to evaluate the nutritional value of the root and leaves of cassava (Manihot sculenta) for juveniles of Nile tilapia (Oreochromis niloticus). Three diets were prepared, a reference and two test diets. The first tested diet contained 50.0% of cassava root and 50.0% of reference diet and the second one consisted of 30.0% of cassava leaf meal and 70.0% of reference diet. Moreover, in every diet was added 0.1% chromium oxide-III (Cr2O3) as inert marker. Sixty juveniles (100.0 +/- 9.0 g) were accommodated in cages (10 fish/cage) for feeding and feces collection. During the day these cages were maintained in a feeding tank (250 L), one tank for each treatment, where they were fed until apparent satiation. After the aforementioned feeding period they were transferred to a fecal collection tank, where they remained until next morning. The collected feces were frozen and dried for analyzes. The apparent digestibility coefficients (ADC) were calculated on basis of Cr2O3 concentration present in diets and feces. The ADC of reference diet for DM, cassava leaf and root were, respectively 85.23%, 81.22% and 91.44%; CP to 97.35%, 73.37% and 91.46% and for the GE to 87.70%, 64.70% and 92.20%, the values obtained for the diet with cassava root significantly higher (P<0.05). Summarizing, root and cassava leaves can be used as alternative ingredients for compose balanced diets for Nile tilapia juveniles.

Low-level laser therapy (670 nm) on viability of random skin flap in rats

This study investigated the effects of 670 nm laser, at different fluences, on the viability of skin flap in rats. One hundred male animals were used. The animals were divided into control group; group treated with 3 J/cm(2); group treated with 6 J/cm(2); group treated with 12 J/cm(2) and group treated with 24 J/cm(2). The skin flap was made on the backs of all animals studied, with a plastic sheet interposed between the flap and the donor site. Laser irradiation was done immediately after the surgery and on days 1, 2, 3 and 4 after surgery. The percentage of necrosis of the flap was calculated at the 7th postoperative day. Additionally, a sample of each flap was collected to enable us to count the blood vessels. Treated animals showed a statistically significant smaller area of necrosis than did the control group. The necrosis in the treated groups was 41.82% (group 2), 36.51% (group 3), 29.45% (group 4) and 20.37% (group 5). We also demonstrated that laser irradiation at 670 nm, at all doses used, had a stimulatory effect on angiogenesis. Our study showed that the 670 nm laser was efficient to increase the viability of the skin flap, at all fluences used, with a tendency of reaching better results at higher doses.

Individual Specialization in the Hunting-wasp Trypoxylon (Trypargilum) agamemnon Richards (Hymenoptera: Crabronidae)

Renan B. Pitilin, Marcio S. Araujo, and Maria L.T. Buschini (2012) Individual specialization in the hunting-wasp Trypoxylon (Trypargilum) agamemnon Richards (Hymenoptera: Crabronidae). Zoological Studies 51(5): 655-662. Individuals of a population may differ with respect to resource use. This among-individual variation in resource utilization is called 'individual specialization' and may substantially impact the ecological and evolutionary dynamics of a population. The aim of this study was to evaluate whether females of 1 population of the hunting-wasp Trypoxylon agamemnon differed in their preferences for spider size and/or taxa. To observe the behavior of wasps, trap-nests were installed in an araucaria forest fragment in the Parque Municipal das Araucarias, Guarapuava (PR), southern Brazil. The indices within-individual component (WIC)/total niche width of a population (TNW) and average of values of the proportional similarity index (IS) were used to measure the degree of individual specialization. We found evidence of strong, significant individual specialization in T agamemnon in terms of both prey size (WIC/TNW = 0.43) and taxa (IS = 0.45). We hypothesized that individual specialization in this species resulted from cognitive tradeoffs that limit individuals to exploring a small subset of available resources. http://zoolstud.sinica.edu.tw/Journals/51.5/655.pdf

Reproductive aspects of Harttia carvalhoi Miranda Ribeiro, 1939, a small loricariid from streams of serra da Mantiqueira eastern, SP, Brazil

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

Avaliação audiológica em pacientes portadores de hipotireoidismo

Surdez no hipotireoidismo já foi descrita por diversos autores, porém a fisiopatologia é incerta. OBJETIVOS: Realizar avaliações audiológicas de pacientes com hipotireoidismo adquirido. MATERIAL E MÉTODOS: Grupos de estudo: hipotireoidismo (GH, n-30) e controle (GC, n-30). Parâmetros estudados: gênero, tempo do hipotireoidismo, co-morbidades, sintomas cócleo-vestibulares, exames bioquímicos e hormonais, limiares audiométricos, PEATE e EOAT. RESULTADOS: Todos os participantes eram mulheres; em GH 70% dos pacientes apresentavam tireoidite de Hashimoto e 60% tinham diagnóstico de hipotireoidismo há mais de 5 anos. Depressão e hipertensão foram as principais co-morbidades do grupo GH. Todos os pacientes de GH tinham valores elevados de TSH e 50% deles apresentavam diminuição de T4 livre. Surdez neurossensorial foi detectada em 22 orelhas de GH e em 7 de GC. PEATE mostrou-se normal nos participantes do GC e alterado em 10 orelhas do GH, havendo predomínio do aumento de L-V. EOAT estiveram ausentes em 12 orelhas de GH e em 4 de GC. CONCLUSÕES: Os pacientes com hipotireoidismo apresentaram mais sintomas cócleo-vestibulares, limiares audiométricos mais elevados, prolongamento das latências absolutas de L-V no PEATE e ausência ou redução as amplitudes das emissões otoacústicas. Tais alterações não estavam associadas aos níveis de TSH e T4 livre.

Ácaros predadores associados ao ácaro-da-erinose da lichia

O objetivo deste trabalho foi identificar ácaros predadores em plantas de lichia e correlacionar o desenvolvimento populacional dessas espécies com o do ácaro-da-erinose da lichia, Aceria litchii. A pesquisa foi desenvolvida no Município de Casa Branca, SP, com árvores adultas, de 12 anos de idade, da variedade Bengal. Mensalmente, de agosto de 2008 a setembro de 2009, foram coletadas folhas para avaliação dos níveis populacionais de A. litchii e de ácaros predadores. Foram registrados 6.557 indivíduos da família Phytoseiidae. A espécie mais abundante foi Amblyseius compositus (42,6%), seguida por Phytoseius intermedius (31,2%), Euseius concordis (14,1%), Amblyseius herbicolus (8,8%) e Iphiseiodes zuluagai (3,3%). O desenvolvimento populacional de A. compositus, E. concordis e I. zuluagai correlacionou-se positivamente com o de Aceria litchii, o que indica relação de predação.