Gemini Observations of Disks and Jets in Young Stellar Objects and in Active Galaxies

We present first results from the Near-infrared Integral Field Spectrograph (NIFS) located at Gemini North. For the active galaxies Cygnus A and Perseus A we observe rotationally-supported accretion disks and adduce the existence of massive central black holes and estimate their masses. In Cygnus A we also see remarkable high-excitation ionization cones dominated by photoionization from the central engine. In the T-Tauri stars HV Tau C and DG Tau we see highly-collimated bipolar outflows in the [Fe II] 1.644 micron line, surrounded by a slower molecular bipolar outflow seen in the H_2 lines, in accordance with the model advocated by Pyo et al. (2002).Comment: Invited paper presented at the 5th Stromlo Symposium. 9 pages, 7 figures. Accepted for publication in Astrophysics & Space Scienc

The Physics of turbulent and dynamically unstable Herbig-Haro jets

The overall properties of the Herbig-Haro objects such as centerline velocity, transversal profile of velocity, flow of mass and energy are explained adopting two models for the turbulent jet. The complex shapes of the Herbig-Haro objects, such as the arc in HH34 can be explained introducing the combination of different kinematic effects such as velocity behavior along the main direction of the jet and the velocity of the star in the interstellar medium. The behavior of the intensity or brightness of the line of emission is explored in three different cases : transversal 1D cut, longitudinal 1D cut and 2D map. An analytical explanation for the enhancement in intensity or brightness such as usually modeled by the bow shock is given by a careful analysis of the geometrical properties of the torus.Comment: 17 pages, 10 figures. Accepted for publication in Astrophysics & Spac

Extragalactic jets on subpc and large scales

Jets can be probed in their innermost regions (d~0.1 pc) through the study of the relativistically-boosted emission of blazars. On the other extreme of spatial scales, the study of structure and dynamics of extragalactic relativistic jets received renewed impulse after the discovery, made by Chandra, of bright X-ray emission from regions at distances larger than hundreds of kpc from the central engine. At both scales it is thus possible to infer some of the basic parameters of the flow (speed, density, magnetic field intensity, power). After a brief review of the available observational evidence, I discuss how the comparison between the physical quantities independently derived at the two scales can be used to shed light on the global dynamics of the jet, from the innermost regions to the hundreds of kpc scale.Comment: Proceedings of the 5th Stromlo Symposium: Disks, Winds, and Jets - from Planets to Quasars. Accepted, to be published in Astrophysics & Space Scienc

Factors Associated with Revision Surgery after Internal Fixation of Hip Fractures

Background: Femoral neck fractures are associated with high rates of revision surgery after management with internal fixation. Using data from the Fixation using Alternative Implants for the Treatment of Hip fractures (FAITH) trial evaluating methods of internal fixation in patients with femoral neck fractures, we investigated associations between baseline and surgical factors and the need for revision surgery to promote healing, relieve pain, treat infection or improve function over 24 months postsurgery. Additionally, we investigated factors associated with (1) hardware removal and (2) implant exchange from cancellous screws (CS) or sliding hip screw (SHS) to total hip arthroplasty, hemiarthroplasty, or another internal fixation device. Methods: We identified 15 potential factors a priori that may be associated with revision surgery, 7 with hardware removal, and 14 with implant exchange. We used multivariable Cox proportional hazards analyses in our investigation. Results: Factors associated with increased risk of revision surgery included: female sex, [hazard ratio (HR) 1.79, 95% confidence interval (CI) 1.25-2.50; P = 0.001], higher body mass index (fo

Tendências no desenvolvimento de gases de proteção utilizados na soldagem MIG/MAG Trends in the development of protective gases used in GMAW welding

Este trabalho tem como objetivo apresentar uma revisão do estado da arte sobre os gases de proteção usados nos processos de soldagem a arco elétrico, com ênfase na soldagem MIG/MAG do aço. São apresentados os principais conceitos da física do arco e as propriedades relacionadas aos gases de proteção. O modelo de atmosfera ligeiramente oxidante para os gases de proteção é discutido, sendo mostradas as formulações dos gases estudados em artigos científicos e em patentes depositadas, bem como as reivindicações (vantagens) requeridas. Também são mencionados alguns poucos estudos usando adições de gases não convencionais. Foi observado que no desenvolvimento de gases de proteção para soldagem MIG/MAG do aço predomina o modelo da formação de atmosfera ligeiramente oxidante. A maioria das formulações propostas envolve o uso de misturas binárias, ternárias e até quaternárias dos gases Ar, He, CO2 e O2. Em aplicações específicas, adições de N2 e H2 foram usadas. Neste sentido, pouca inovação foi identificada, sendo atribuídas possíveis razões a este fato. A tendência observada para o desenvolvimento de gases de proteção parece ser o uso de misturas ricas em gases inertes, com adições calibradas de elementos oxidantes, sempre atendendo a aplicações específicas.<br>This paper has as objective to present a state of the art review on the shielding gases used in the electric arc welding processes, with emphasis on GMAW welding of steel. There are shown the main concepts of arc physics and properties related to shielding gases. The model of slightly oxidizing atmosphere for shielding gases is discussed, and the formulations of the gases studied in scientific articles and in deposited patents, as well as the claims (benefits) required. It also mentions some few studies using additions of non-conventional gases. It was observed that for the development of shielding gases for the GMAW steel welding the model of slightly oxidizing atmosphere is predominant. Most of proposed formulations involve the use of binary, ternary or even quaternary mixtures of the gases Ar, He, CO2 and O2. For specific aplications, additions of N2 e H2 were used. In this meaning, few innovations were identified, and possible reasons were attributed. The trend observed for the development of shielding gases seems to be the use of mixtures rich in inert gases, with calibrated additions of oxidizing elements, always looking for specific applications