Search results for "bula"

showing 10 items of 1798 documents

How common is isolated nocturnal hypertension?

2020

The growing use of methods to measure blood pressure (BP) under everyday life conditions in ‘out-of-office’ settings, through either 24-h ambulatory BP monitoring (ABPM) or home BP monitoring (HBPM), for defining BP status has led to identification of four specific hypertension phenotypes, characterized by variable agreement or disagreement between office BP (OBP) and out-of-office BP: true normotension (normal office and out-of-office BP), sustained hypertension (both elevated office and out-of-office BP), masked hypertension (normal office BP and out-of-office BP), and white-coat hypertension (WCH), when OBP is elevated, but out-of-office BP levels are within normal limits. The term ‘whit…

Settore MED/14 - Nefrologiamedicine.medical_specialtySettore MED/09 - Medicina InternaPhysiologybusiness.industryMEDLINECardiologyBlood PressureBlood Pressure DeterminationNocturnalambulatory blood pressure monitoring - Home blood pressure - Nocturnal hypertension - Masked hypertensionBlood pressureInternal medicineHypertensionInternal MedicinemedicineCardiologyPrevalenceHumansCardiology and Cardiovascular Medicinebusiness
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Manual therapy of the mandibular accessory ligaments for the management of temporomandibular joint disorders.

2011

Temporomandibular joint disorders are characterized by chronic or acute musculoskeletal or myofascial pain with dysfunction of the masticatory system. Treatment modalities include occlusal splints, patient education, activity modification, muscle and joint exercises, myofascial therapy, acupuncture, and manipulative therapy. In the physiology of the temporomandibular joint, accessory ligaments limit the movement of the mandible. A thorough knowledge of the anatomy of accessory ligaments is necessary for good clinical management of temporomandibular joint disorders. Although general principles regarding the anatomy of the ligaments are relatively clear, very little substantiated information …

Settore MED/28 - Malattie OdontostomatologicheLigaments ArticularHumansMandibleTemporomandibular Joint DisordersManipulation OsteopathicHumanThe Journal of the American Osteopathic Association
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IMAGING OF VESTIBULAR SCHWANNOMA [Chapter 4]

2020

Lesions of the cerebellopontine angle and internal auditory canal are a frequent finding in neuroradiological examinations and their detection may represent a diagnostic challenge. Among these lesions, vestibular schwannomas and meningiomas are certainly the most frequent and account for up to 90% of all cerebellopontine angle tumours. The remaining ones are a group of lesions arising from the different structures found in these anatomical regions such as haemangiomas, lipomas, lymphomas, facial nerve tumours, and aneurysms. This chapter will introduce this topic focusing on a practical coverage of the typical and atypical neuroradiological signs that will drive towards the most correct dif…

Settore MED/37 - Neuroradiologiavestibular schwannomas cerebellopontine angle differential diagnosis neuroimaging CT MRISettore MED/36 - Diagnostica Per Immagini E Radioterapia
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La nuova Legge Italiana sull'infibulazione. Aspetti medico-legali

2014

Settore MED/43 - Medicina LegaleInfibulazione mutilazioni genitali femminili lesioni personali
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Immediate bleeding complications in dental implants: A systematic review

2014

Objective: A review is made of the immediate or immediate postoperative bleeding complications in dental implants, with a view to identifying the areas of greatest bleeding risk, the causes of bleeding, the length of the implants associated with bleeding, the most frequently implicated blood vessels, and the treatments used to resolve these complications. Material and Methods: A Medline (PubMed) and Embase search was made of articles on immediate bleeding complications in dental implants published in English up until May 2014. Inclusion criteria: studies in humans subjects with severe bleeding immediately secondary to implant placement, which reported the time until the hemorrhage, the impl…

Severe bleedingmedicine.medical_specialtyTime Factorsmedicine.medical_treatmentPerforation (oil well)DentistryOdontologíaReviewPostoperative HemorrhageAnticoagulation TreatmentMandibular caninemedicineIntubationHumansGeneral DentistryDental Implantsbusiness.industry:CIENCIAS MÉDICAS [UNESCO]Ciencias de la saludSurgeryImplant placementOtorhinolaryngologyUNESCO::CIENCIAS MÉDICASSurgeryImplantOral SurgerybusinessAirwayMedicina Oral, Patología Oral y Cirugía Bucal
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AE Aurigae: First detection of non-thermal X-ray emission from a bow shock produced by a runaway star

2012

Runaway stars produce shocks when passing through interstellar medium at supersonic velocities. Bow shocks have been detected in the mid-infrared for several high-mass runaway stars and in radio waves for one star. Theoretical models predict the production of high-energy photons by non-thermal radiative processes in a number sufficiently large to be detected in X-rays. To date, no stellar bow shock has been detected at such energies. We present the first detection of X-ray emission from a bow shock produced by a runaway star. The star is AE Aur, which was likely expelled from its birthplace due to the encounter of two massive binary systems and now is passing through the dense nebula IC 405…

Shock waveAstrofísicaCiencias Astronómicasstars: kinematics and dynamicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsX-rays: generalISM: cloudsmassive [stars]general [X-rays]Radiative transferISM: clouds radiation mechanisms: non-thermal stars: individual: AE Aur stars: kinematics and dynamics stars: massive X-rays: generalAstrophysics::Solar and Stellar AstrophysicsBow shock (aerodynamics)kinematics and dynamics [stars]Solar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsCosmic dustPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)NebulaAstronomy and Astrophysicsradiation mechanisms: non-thermalnon-thermal [radiation mechanisms]Astrophysics - Astrophysics of GalaxiesInterstellar mediumAstronomíastars: individual (AE Aur)stars: massiveStarsindividual (AE Aur) [stars]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomenaclouds [ISM]Radio wave
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3D MHD modeling of the expanding remnant of SN 1987A : role of magnetic field and non-thermal radio emission

2018

Aims. We investigate the role played by a pre-supernova (SN) ambient magnetic field on the dynamics of the expanding remnant of SN 1987A and the origin and evolution of the radio emission from the remnant, in particular, during the interaction of the blast wave with the nebula surrounding the SN. Methods. We model the evolution of SN 1987A from the breakout of the shock wave at the stellar surface to the expansion of its remnant through the surrounding nebula by 3D MHD simulations. The model considers the radiative cooling, the deviations from equilibrium of ionization, the deviation from temperature-equilibration between electrons and ions, and a plausible configuration of the pre-SN ambie…

Shock waveH II regionMagnetohydrodynamics (MHD)shock waveAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesField strengthISM [radio continuum]AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesmagnetohydrodynamics (MHD)Radio spectrumindividual: SN 1987A [supernovae]0103 physical sciencesISM [X-rays]010303 astronomy & astrophysicsBlast waveISM: supernova remnantAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Nebulasupernovae: individual: SN 1987A010308 nuclear & particles physicssupernova remnants [ISM]Astronomy and Astrophysicsshock wavesX-rays: ISMMagnetic fieldradio continuum: ISMSpace and Planetary ScienceMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena
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Supernova 1987A: a Template to Link Supernovae to their Remnants

2015

The emission of supernova remnants reflects the properties of both the progenitor supernovae and the surrounding environment. The complex morphology of the remnants, however, hampers the disentanglement of the two contributions. Here we aim at identifying the imprint of SN 1987A on the X-ray emission of its remnant and at constraining the structure of the environment surrounding the supernova. We performed high-resolution hydrodynamic simulations describing SN 1987A soon after the core-collapse and the following three-dimensional expansion of its remnant between days 1 and 15000 after the supernova. We demonstrated that the physical model reproducing the main observables of SN 1987A during …

Shock wavesupernovae: individual (SN 1987A)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsPower lawSpectral lineGravitational collapseAstrophysics::Solar and Stellar AstrophysicsHydrodynamics instabilities ISM: supernova remnants shock waves supernovae: individual (SN 1987A) X-rays: ISM.EjectaAstrophysics::Galaxy AstrophysicsISM: supernova remnantsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsNebulaAstronomy and AstrophysicsObservableshock wavesX-rays: ISMhydrodynamics instabilities ISM: supernova remnants shock waves supernovae: individual: SN 1987A X-rays: ISMSupernovainstabilitiesSpace and Planetary ScienceHydrodynamicsAstrophysics - High Energy Astrophysical Phenomena
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Validation of the use of Actigraph GT3X accelerometers to estimate energy expenditure in full time manual wheelchair users with spinal cord injury.

2013

Study design: Cross-sectional validation study. Objectives: The goals of this study were to validate the use of accelerometers by means of multiple linear models (MLMs) to estimate the O2 consumption (VO2) in paraplegic persons and to determine the best placement for accelerometers on the human body. Setting: Non-hospitalized paraplegics’ community. Methods: Twenty participants (age=40.03 years, weight=75.8 kg and height=1.76 m) completed sedentary, propulsion and housework activities for 10 min each. A portable gas analyzer was used to record VO2. Additionally, four accelerometers (placed on the non-dominant chest, non-dominant waist and both wrists) were used to collect second-by-second a…

Signal processingAdultMalemedicine.medical_specialtyPercentileMean squared errormedia_common.quotation_subjectPopulationMonitoring AmbulatoryAccelerometerModels BiologicalAccelerationPhysical medicine and rehabilitationOxygen ConsumptionAccelerometrymedicineEvaluation methodologyHumanseducationSpinal Cord Injuriesmedia_commonParaplegiaeducation.field_of_studyVariablesbusiness.industryPhysical activityLinear modelGeneral MedicineMiddle AgedGas analyzerAccelerometerCross-Sectional StudiesNeurologyWheelchairsFemaleNeurology (clinical)businessMATEMATICA APLICADAEnergy MetabolismSpinal cord
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Active unilateral condylar hyperplasia : assessment of the usefulness of single photon emission computed tomography

2020

[Background] This study aims to evaluate whether the uptake difference by the condyles evaluated using single photon emission computed tomography (SPECT) examination is useful for predicting the activity of the feature and the advance of this pathology.

Single photon emission computed tomographyCondylar hyperplasiaMandibleSingle-photon emission computed tomographyTemporomandibular jointCondyleMedicineHumansClinical significanceProspective StudiesFacial asymmetryGeneral DentistryTomography Emission-Computed Single-PhotonHyperplasiamedicine.diagnostic_testbusiness.industryResearchMandibular CondyleScintigra-phyCraniometry:CIENCIAS MÉDICAS [UNESCO]ScintigraphyTemporomandibular jointmedicine.anatomical_structureOtorhinolaryngologyUNESCO::CIENCIAS MÉDICASBone maturationSurgeryTomographyOral SurgeryNuclear medicinebusinessFacial symmetry
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