Microquasar models for 3EG J1828+0142 and 3EG J1735-1500

Microquasars are promising candidates to emit high-energy gamma-rays. Moreover, statistical studies show that variable EGRET sources at low galactic latitudes could be associated with the inner spiral arms. The variable nature and the location in the Galaxy of the high-mass microquasars, concentrated in the galactic plane and within 55 degrees from the galactic center, give to these objects the status of likely counterparts of the variable low-latitude EGRET sources. We consider in this work the two most variable EGRET sources at low-latitudes: 3EG J1828+0142 and 3EG J1735-1500, proposing a microquasar model to explain the EGRET data in consistency with the observations at lower energies (from radio frequencies to soft gamma-rays) within the EGRET error box.

Radio continuum and near-infrared study of the MGRO J2019+37 region

MGRO J2019+37 is an unidentified extended source of very high energy gamma-rays originally reported by the Milagro Collaboration as the brightest TeV source in the Cygnus region. Its extended emission could be powered by either a single or several sources. The GeV pulsar AGL J2020.5+3653 , discovered by AGILE and associated with PSR J2021+3651 , could contribute to the emission from MGRO J2019+37 . Aims. Our aim is to identify radio and near-infrared sources in the field of the extended TeV source MGRO J2019+37 , and study potential counterparts to explain its emission. Methods. We surveyed a region of about 6 square degrees with the Giant Metrewave Radio Telescope (GMRT) at the frequency 610 MHz. We also observed the central square degree of this survey in the near-infrared -band using the 3.5 m telescope in Calar Alto. Archival X-ray observations of some specific fields are included. VLBI observations of an interesting radio source were performed. We explored possible scenarios to produce the multi-TeV emission from MGRO J2019+37 and studied which of the sources could be the main particle accelerator. Results. We present a catalogue of 362 radio sources detected with the GMRT in the field of MGRO J2019+37 , and the results of a cross-correlation of this catalog with one obtained at near-infrared wavelengths, which contains ~3105 sources, as well as with available X-ray observations of the region. Some peculiar sources inside the ~1° uncertainty region of the TeV emission from MGRO J2019+37 are discussed in detail, including the pulsar PSR J2021+3651 and its pulsar wind nebula PWN G75.2+0.1 , two new radio-jet sources, the H II region Sh 2-104 containing two star clusters, and the radio source NVSS J202032+363158 . We also find that the hadronic scenario is the most likely in case of a single accelerator, and discuss the possible contribution from the sources mentioned above. Conclusions. Although the radio and GeV pulsar PSR J2021+3651 / AGL J2020.5+3653 and its associated pulsar wind nebula PWN G75.2+0.1 can contribute to the emission from MGRO J2019+37 , extrapolation of the GeV spectrum does not explain the detected multi-TeV flux. Other sources discussed here could contribute to the emission of the Milagro source.

Observation of Pulsed γ-Rays Above 25 GeV from the Crab Pulsar with MAGIC

One fundamental question about pulsars concerns the mechanism of their pulsed electromagnetic emission. Measuring the high-end region of a pulsar's spectrum would shed light on this question. By developing a new electronic trigger, we lowered the threshold of the Major Atmospheric γ-ray Imaging Cherenkov (MAGIC) telescope to 25 giga-electron volts. In this configuration, we detected pulsed γ-rays from the Crab pulsar that were greater than 25 giga-electron volts, revealing a relatively high cutoff energy in the phase-averaged spectrum. This indicates that the emission occurs far out in the magnetosphere, hence excluding the polar-cap scenario as a possible explanation of our measurement. The high cutoff energy also challenges the slot-gap scenario.

Improving the performance of the single-dish Cherenkov telescope MAGIC through the use of signal timing

The Cherenkov light flashes produced by Extensive Air Showers are very short in time. A high bandwidth and fast digitizing readout, therefore, can minimize the influence of the background from the light of the night sky, and improve the performance in Cherenkov telescopes. The time structure of the Cherenkov image can further be used in single-dish Cherenkov telescopes as an additional parameter to reduce the background from unwanted hadronic showers. A description of an analysis method which makes use of the time information and the subsequent improvement on the performance of the MAGIC telescope (especially after the upgrade with an ultra fast 2 GSamples/s digitization system in February 2007) will be presented. The use of timing information in the analysis of the new MAGIC data reduces the background by a factor two, which in turn results in an enhancement of about a factor 1.4 of the flux sensitivity to point-like sources, as tested on observations of the Crab Nebula.

Optimized dark matter searches in deep observations of Segue 1 with MAGIC

We present the results of stereoscopic observations of the satellite galaxy Segue 1 with the MAGIC Telescopes, carried out between 2011 and 2013. With almost 160 hours of good-quality data, this is the deepest observational campaign on any dwarf galaxy performed so far in the very high energy range of the electromagnetic spectrum. We search this large data sample for signals of dark matter particles in the mass range between 100 GeV and 20 TeV. For this we use the full likelihood analysis method, which provides optimal sensitivity to characteristic gamma-ray spectral features, like those expected from dark matter annihilation or decay. In particular, we focus our search on gamma-rays produced from different final state Standard Model particles, annihilation with internal bremsstrahlung, monochromatic lines and box-shaped signals. Our results represent the most stringent constraints to the annihilation cross-section or decay lifetime obtained from observations of satellite galaxies, for masses above few hundred GeV. In particular, our strongest limit (95% confidence level) corresponds to a ~ 500 GeV dark matter particle annihilating into τ+τ−, and is of order langleσannvrangle simeq 1.2 × 10−24 cm3 s−1 a factor ~ 40 above the langleσannvrangle simeq thermal value.

Estudo morfométrico do coração fetal: sua utilização como parâmetro para análise ecocardiográfica

OBJETIVO: Avaliar o diâmetro, o perímetro e a área das valvas atrioventriculares do coração fetal, bem como a espessura das paredes ventriculares e os diâmetros das cavidades ventriculares. MATERIAIS E MÉTODOS: Foram dissecados 20 corações de fetos com idade gestacional entre 28 e 36 semanas. Em seguida foram medidos os diâmetros ântero-posterior e transverso e aferidos as áreas e os perímetros das valvas mitral e tricúspide, bem como foram medidas as espessuras das paredes ventriculares e os diâmetros de suas cavidades, utilizando-se um paquímetro com acurácia de1/10 mm. RESULTADOS: Os diâmetros ântero-posterior e transverso da valva atrioventricular esquerda mediram, em média, 10,35 ± 1,62 mm e 9,90 ± 1,79 mm, respectivamente, e os diâmetros ântero-posterior e transverso da valva atrioventricular direita, 10,98 ± 1,90 mm e 9,51 ± 1,81 mm, respectivamente. A área e o perímetro da valva mitral foram de 84,06 ± 25,09 mm² e 29,87 ± 3,96 mm, respectivamente. A área e o perímetro da valva tricúspide mediram, respectivamente, 84,49 ± 26,79 mm² e 28,44 ± 3,85 mm. No ventrículo direito a espessura da parede anterior foi de 5,00 ± 1,70 mm e a da parede posterior foi de 3,83 ± 0,91 mm; no ventrículo esquerdo a espessura da parede anterior foi de 4,25 ± 0,87 mm e a da parede posterior foi de 4,14 ± 0,89 mm. O septo interventricular teve espessura de 4,10 ± 1,13 mm. O ventrículo direito teve como diâmetro ântero-posterior 9,25 ± 0,85 mm, e como diâmetro transverso 8,24 ± 0,42 mm. O ventrículo esquerdo mediu 9,95 ± 0,37 mm para o diâmetro ântero-posterior e 9,20 ± 0,40 mm para o diâmetro transverso. CONCLUSÃO: O conhecimento dos dados morfométricos do coração do feto é de grande importância para o diagnóstico ecocardiográfico de possíveis malformações cardíacas.

Eficacia analgésica del diclofenaco sódico vs. ibuprofeno después de la extracción quirúrgica de un tercer molar inferior incluido

Objetivo: En este estudio evaluamos la eficacia analgésica del diclofenaco sódico en comparación con el ibuprofeno, después de la extracción quirúrgica de un tercer molar inferior incluido. Diseño de estudio: Los pacientes que participaron en el estudio fueron distribuidos de forma aleatoria en dos grupos. Uno fue el grupo ibuprofeno y el otro el grupo diclofenaco. La intervención practicada fue la extracción quirúrgica de un tercer molar inferior cuya dificultad fue determinada en función del grado de inclusión en todos los pacientes. Las variables registradas fueron la intensidad del dolor y la necesidad de medicación de rescate durante un periodo de una semana. Los registros se realizaron una vez al día a la misma hora y registrados en un cuaderno por parte del paciente. Resultados: Un total de 81 pacientes (87.1%) fueron incluidos en el estudio. Los valores fueron similares en las primeras 48 horas postoperatorias, pero a partir del tercer día existió una tendencia del grupo diclofenaco a mostrar valores de dolor superiores, aunque sin llegar a existir diferencias estadísticamente significativas (p>0.05). Esta tendencia a presentar mayor dolor durante el periodo postoperatorio en el grupo diclofenaco también se vio reflejada en el requerimiento del analgésico de rescate y en el número de comprimidos empleados. Conclusiones: No se evidenciaron diferencias estadísticamente significativas en cuanto a la eficacia analgésica del diclofenaco sódico respecto al ibuprofeno, aunque sí pudo observarse una mayor tendencia hacia la necesidad de más medicación suplementaria durante los 2 primeros días del postoperatorio en el grupo diclofenaco pero sin adquirir significación estadística (p>0.05).

The Coordinated Radio and Infrared Survey for High-mass Star Formation. II. Source Catalog

The CORNISH project is the highest resolution radio continuum survey of the Galactic plane to date. It is the 5 GHz radio continuum part of a series of multi-wavelength surveys that focus on the northern GLIMPSE region (10° < l < 65°), observed by the Spitzer satellite in the mid-infrared. Observations with the Very Large Array in B and BnA configurations have yielded a 1.''5 resolution Stokes I map with a root mean square noise level better than 0.4 mJy beam 1. Here we describe the data-processing methods and data characteristics, and present a new, uniform catalog of compact radio emission. This includes an implementation of automatic deconvolution that provides much more reliable imaging than standard CLEANing. A rigorous investigation of the noise characteristics and reliability of source detection has been carried out. We show that the survey is optimized to detect emission on size scales up to 14'' and for unresolved sources the catalog is more than 90% complete at a flux density of 3.9 mJy. We have detected 3062 sources above a 7σ detection limit and present their ensemble properties. The catalog is highly reliable away from regions containing poorly sampled extended emission, which comprise less than 2% of the survey area. Imaging problems have been mitigated by down-weighting the shortest spacings and potential artifacts flagged via a rigorous manual inspection with reference to the Spitzer infrared data. We present images of the most common source types found: H II regions, planetary nebulae, and radio galaxies. The CORNISH data and catalog are available online at http://cornish.leeds.ac.uk.

Aspectos tomográficos e anatomopatológicos do padrão de pavimentação em mosaico

OBJETIVO: Relatar os aspectos na tomografia computadorizada de alta resolução de diversas doenças que cursam com o padrão tomográfico de "pavimentação em mosaico". MATERIAIS E MÉTODOS: Foram estudados sete pacientes, com diagnósticos de proteinose alveolar, carcinoma bronquíolo-alveolar, pneumonia lipídica e pneumocistose, e é discutida a correlação dos aspectos tomográficos com os achados anatomopatológicos. RESULTADOS: Nos casos de pneumocistose, os espaços alveolares estavam cheios de material espumoso, no qual eram encontrados parasitas de permeio a surfactante, fibrina e restos celulares. Nos casos de carcinoma bronquíolo-alveolar, os septos estavam espessados por fibrose ou por linfangite associada, com células tumorais revestindo internamente as paredes alveolares, e produção de muco. No paciente com proteinose alveolar foram observados septos espessados por edema, com enchimento alveolar determinado por material lipoproteico. No paciente com aspiração de óleo mineral, os achados histopatológicos foram de espessamento dos septos alveolares determinado por proliferação celular, observando-se vacúolos de gordura no interior dos septos alveolares. CONCLUSÃO: O padrão de pavimentação em mosaico oferece um amplo diagnóstico diferencial, necessitando ser avaliado em conjunto com os dados clínicos.

Achados da tomografia computadorizada de alta resolução na histiocitose de células de Langerhans pulmonar

OBJETIVO: Caracterizar, por meio da tomografia computadorizada de alta resolução, as principais alterações pulmonares da histiocitose de células de Langerhans. MATERIAIS E MÉTODOS: Foram avaliadas, retrospectivamente, as tomografias computadorizadas de alta resolução de oito pacientes com diagnóstico comprovado da doença a partir de biópsia pulmonar a céu aberto, biópsia transbrônquica, estudos de imuno-histoquímica e/ou lesões extrapulmonares associadas. RESULTADOS: Pequenas lesões císticas, arredondadas e de paredes finas foram observadas em todos os pacientes. Nódulos, com distribuição predominantemente periférica no parênquima pulmonar, estavam presentes em 75% dos exames estudados. As lesões apresentaram distribuição difusa, com predomínio nos terços superior e médio dos pulmões em todos os casos, mas acometimento dos recessos costofrênicos foi observado em 25% dos pacientes. CONCLUSÃO: A comparação das tomografias computadorizadas de alta resolução com radiografias de tórax mostrou que cistos de paredes finas e pequenos nódulos não podem ser avaliados satisfatoriamente por radiografias convencionais. A tomografia computadorizada de alta resolução, por sua capacidade de detectar e caracterizar cistos e nódulos pulmonares, permite o diagnóstico de histiocitose de células de Langerhans pulmonar com alta probabilidade.

Espessamento parietal da vesícula biliar no exame ultrassonográfico: como interpretar?

O objetivo desta revisão é fornecer auxílio na interpretação correta do espessamento das paredes da vesícula biliar e seus possíveis diagnósticos diferenciais. O espessamento da vesícula biliar é um achado frequente em exame de ultrassonografia e um tema de grande interesse, por ter sido considerado durante muito tempo como sinal específico de colecistite aguda, apesar de se reconhecer que ocorre em uma série de outras situações clínicas. A adequada caracterização e interpretação desse achado é de grande importância, pois o diagnóstico correto tem impacto direto no tratamento, que em alguns casos inclui intervenção cirúrgica. Neste artigo procuramos apresentar um conjunto de sinais ultrassonográficos que, associados ao quadro clínico e laboratorial do paciente, permitem restringir as alternativas diagnósticas e estabelecer, com maior precisão, a causa do espessamento parietal da vesícula biliar, através de uma avaliação racional dos dados obtidos.

Massive protostars as gamma-ray sources.

Massive protostars have associated bipolar outflows with velocities of hundreds of km s-1. Such outflows can produce strong shocks when they interact with the ambient medium leading to regions of nonthermal radio emission. Aims. We aim at exploring under which conditions relativistic particles are accelerated at the terminal shocks of the protostellar jets and whether they can produce significant gamma-ray emission. Methods. We estimate the conditions necessary for particle acceleration up to very high energies and gamma-ray production in the nonthermal hot spots of jets associated with massive protostars embedded in dense molecular clouds. Results. We show that relativistic bremsstrahlung and proton-proton collisions can make molecular clouds with massive young stellar objects detectable by the Fermi satellite at MeV-GeV energies and by Cherenkov telescope arrays in the GeV-TeV range. Conclusions. Gamma-ray astronomy can be used to probe the physical conditions in star-forming regions and particle acceleration processes in the complex environment of massive molecular clouds.

Randomized, crossover, double-blind, placebo-controlled trial to assess the lipid lowering effect of co-formulated TDF/FTC

Abstract INTRODUCTION: Previous studies have described improvements on lipid parameters when switching from other antiretroviral drugs to tenofovir (TDF) and impairments in lipid profile when discontinuing TDF. [1-3] It is unknown, however, if TDF has an intrinsic lipid-lowering effect or such findings are due to the addition or removal of other offending agents or other reasons. MATERIALS AND METHODS: RESULTS: 46 subjects with a median age of 43 (40-48) years were enrolled in the study: 70% were male, 56% received DRV/r and 44% LPV/r. One subject withdrew the study voluntarily at week 4 and another one interrupted due to diarrhoea at week 24. Treatment with TDF/FTC decreased total, LDL and HDL-cholesterol from 235.9 to 204.9 (p<0.001), 154.7 to 127.6 (p<0.001) and 50.3 to 44.5 mg/dL (p<0.001), respectively. In comparison, total, LDL and HDL-cholesterol levels remained stable during placebo exposure. Week 12 total cholesterol (p<0.001), LDL-cholesterol (p<0.001) and HDL-cholesterol (p=0.011) levels were significantly lower in TDF/FTC versus placebo. Treatment with TDF/FTC reduced the fraction of subjects with abnormal fasting total-cholesterol (≥200 mg/dL) from 86.7% to 56.8% (p=0.001) and LDL-cholesterol (≥130 mg/dL) from 87.8% to 43.9% (p<0.001), which was not observed with placebo. There were no virological failures, and CD4 and triglyceride levels remained stable regardless of exposure. CONCLUSION: Coformulated TDF/FTC has an intrinsic lipid-lowering effect, likely attributable to TDF.

Aprenentatge sobre les emocions: la seva influència en l'aprenentage sobre habilitats socials. Desenvolupament i anàlisi d'una intervenció en una aula de P3

Amb aquest treball es pretén comprovar, si l’aplicació d’un conjunt d’activitats dirigides a treballar les emocions, millora les habilitats socials dels alumnes d’Educació Infantil. En primer lloc, es presenta un marc teòric basat en les aportacions i els descobriments de diferents autors sobre diversos aspectes relacionats amb les emocions i, sobre la importància de crear un bon clima dins d’una aula. Posteriorment es presenta el desenvolupament de les activitats que s’han posat en pràctica a l’aula. Per últim, es fa un anàlisi de les dades recollides en aquest estudi i se’n mostren els resultats i les conclusions que s’han extret.

Hints for a fast precessing relativistic radio jet in LS I + 61° 303

Here we discuss two consecutive MERLIN observations of the X-ray binary LS I +61° 303 . The first observation shows a double-sided jet extending up to about 200 AU on both sides of a central source. The jet shows a bent S-shaped structure similar to the one displayed by the well-known precessing jet of SS 433 . The precession suggested in the first MERLIN image becomes evident in the second one, showing a one-sided bent jet significantly rotated with respect to the jet of the day before. We conclude that the derived precession of the relativistic (beta=0.6) jet explains puzzling previous VLBI results. Moreover, the fact that the precession is fast could be the explanation of the never understood short term (days) variability of the associated gamma-ray source 2CG 135+01 / 3EG J0241+6103