Search results for "Non-thermal"

showing 10 items of 33 documents

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
researchProduct

Observational constraints on the modelling of SN 1006

2011

supernova remnantsISM: individual: SN 1006radiation mechanisms: non-thermalacceleration of particlecosmic ray
researchProduct

Long-term monitoring of mrk 501 for its very high energy γ emission and a flare in 2011 october

2012

"As one of the brightest active blazars in both X-ray and very high energy γ -ray bands, Mrk 501, is very useful for" "physics associated with jets from active galactic nuclei. The ARGO-YBJ experiment has monitored Mrk 501 for γ - rays above 0.3 TeV since 2007 November. The largest flare since 2005 was observed from 2011 October and lasted until about 2012 April. In this paper, a detailed analysis of this event is reported. During the brightest γ -ray flaring episodes from 2011 October 17 to November 22, an excess of the event rate over 6σ is detected by ARGO-YBJ in the direction of Mrk 501, corresponding to an increase of the γ -ray flux above 1 TeV by a factor of 6.6 ± 2.2 from its steady…

Active galactic nucleusactive" ["galaxies]Astrophysics::High Energy Astrophysical PhenomenaFluxAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesSpectral linelaw.inventionlaw0103 physical sciencesBlazar010303 astronomy & astrophysicsPhysicsindividual (Markarian 501) – galaxies: active – gamma rays: general – radiation mechanisms: non-thermal [BL Lacertae objects]" "general" ["gamma rays]010308 nuclear & particles physicsBL Lacertae objects: individual (Markarian 501) – galaxies: active – gamma rays: general – radiation mechanisms: non-thermalSettore FIS/01 - Fisica SperimentaleAstronomy and AstrophysicsQuasarGalaxyindividual (Markarian 501)" ["BL Lacertae objects]13. Climate actionSpace and Planetary ScienceSpectral energy distributionFlare
researchProduct

3D simulations of wind-jet interaction in massive X-ray binaries

2010

High-mass microquasars may produce jets that will strongly interact with surrounding stellar winds on binary system spatial scales. We study the dynamics of the collision between a mildly relativistic hydrodynamical jet of supersonic nature and the wind of an OB star. We performed numerical 3D simulations of jets that cross the stellar wind with the code Ratpenat. The jet head generates a strong shock in the wind, and strong recollimation shocks occur due to the initial overpressure of the jet with its environment. These shocks can accelerate particles up to TeV energies and produce gamma-rays. The recollimation shock also strengthens jet asymmetric Kelvin-Helmholtz instabilities produced i…

X-rays : binaries; ISM: jets and outflows; Stars : winds outflows; Radiation mechanisms: non-thermalAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)Astrophysics:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Fuentes de Rayos X [UNESCO]UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Fuentes de Rayos Xwinds outflows [Stars]Supersonic speedAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)non-thermal [Radiation mechanisms]Shock (fluid dynamics)OB starjets and outflows [ISM]Astronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesOverpressureParticle accelerationDiscontinuity (linguistics)Space and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)binaries [X-rays]High Energy Physics::ExperimentUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::EstrellasAstrophysics - High Energy Astrophysical Phenomena:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Estrellas [UNESCO]Astronomy and Astrophysics
researchProduct

Prompt TeV Emission from Cosmic Rays Accelerated by Gamma Ray Bursts Interacting with Surrounding Stellar Wind

2009

11 pages, 1 figure.--ISI article identifier:000263148600009.-- ArXiv pre-print avaible at:http://arxiv.org/abs/0810.1287

Astrofísicaradiation mechanism: non-thermalMesongamma rays: burstsAstrophysics::High Energy Astrophysical PhenomenaNuclear Theorynon-thermal [radiation mechanism]FOS: Physical sciencesSynchrotron radiationCosmic rayAstrophysicsElectronAstrophysics::Cosmology and Extragalactic AstrophysicsStellar-wind bubbleAstrophysicsHigh Energy Physics - Phenomenology (hep-ph)NeutronNuclear ExperimentPhysicstheory [gamma rays]Astrophysics (astro-ph)Gamma raybursts [gamma rays]Astronomy and Astrophysicsgamma rays: theoryHigh Energy Physics - PhenomenologySpace and Planetary ScienceHigh Energy Physics::ExperimentGamma-ray burst
researchProduct

Internal shocks in relativistic outflows: collisions of magnetized shells

2007

(Abridged): We study the collision of magnetized irregularities (shells) in relativistic outflows in order to explain the origin of the generic phenomenology observed in the non-thermal emission of both blazars and gamma-ray bursts. We focus on the influence of the magnetic field on the collision dynamics, and we further investigate how the properties of the observed radiation depend on the strength of the initial magnetic field and on the initial internal energy density of the flow. The collisions of magnetized shells and the radiation resulting from these collisions are calculated using the 1D relativistic magnetohydrodynamics code MRGENESIS. The interaction of the shells with the externa…

Magnetohydrodynamics (MHD)Lorentz transformationAstrophysics::High Energy Astrophysical PhenomenaNon-thermalFOS: Physical sciencesAstrophysicsAstrophysicsKinetic energyUNESCO::ASTRONOMÍA Y ASTROFÍSICAMagnetohydrodynamics (MHD) ; Radiation mechanisms ; Non-thermal ; galaxies ; Jets ; BL Lacertae objects ; X-rayssymbols.namesakeMagnetizationgalaxiesJetsX-raysRadiation mechanismsPhysicsMagnetic energyInternal energybusiness.industryAstrophysics (astro-ph)Astronomy and Astrophysics:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Computational physicsMagnetic fieldSpace and Planetary SciencesymbolsBL Lacertae objectsMagnetohydrodynamicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniabusinessThermal energy:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
researchProduct

Anomalous transport effects on switching currents of graphene-based Josephson junctions

2017

We explore the effect of noise on the ballistic graphene-based small Josephson junctions in the framework of the resistively and capacitively shunted model. We use the non-sinusoidal current-phase relation specific for graphene layers partially covered by superconducting electrodes. The noise induced escapes from the metastable states, when the external bias current is ramped, give the switching current distribution, i.e. the probability distribution of the passages to finite voltage from the superconducting state as a function of the bias current, that is the information more promptly available in the experiments. We consider a noise source that is a mixture of two different types of proce…

DYNAMICSJosephson effectJosephson junctionsGaussianFOS: Physical sciencesgraphemeBioengineering01 natural sciencesNoise (electronics)Settore FIS/03 - Fisica Della Materia010305 fluids & plasmaslaw.inventionsymbols.namesakelawJosephson junction0103 physical sciencesMesoscale and Nanoscale Physics (cond-mat.mes-hall)Graphene; Josephson junctions; Levy processes; Non-thermal noise; Bioengineering; Chemistry (all); Materials Science (all); Mechanics of Materials; Mechanical Engineering; Electrical and Electronic EngineeringMechanics of MaterialGeneral Materials ScienceElectrical and Electronic Engineering010306 general physicsPhysicsSuperconductivityLevy processesCondensed matter physicsCondensed Matter - Mesoscale and Nanoscale PhysicsGrapheneMechanical EngineeringSTABLE RANDOM-VARIABLESChemistry (all)Non-thermal noiseBiasingGeneral ChemistryGraphene; Josephson junctions; Levy processes; Non-thermal noise; STABLE RANDOM-VARIABLES; DYNAMICSLevy processeMechanics of MaterialsPhysics - Data Analysis Statistics and ProbabilitysymbolsProbability distributionMaterials Science (all)GrapheneTransport phenomenaData Analysis Statistics and Probability (physics.data-an)
researchProduct

The NHXM observatory

2011

Exploration of the X-ray sky has established X-ray astronomy as a fundamental astrophysical discipline. While our knowledge of the sky below 10 keV has increased dramatically (∼8 orders of magnitude) by use of grazing incidence optics, we still await a similar improvement above 10 keV, where to date only collimated instruments have been used. Also ripe for exploration is the field of X-ray polarimetry, an unused fundamental tool to understand the physics and morphology of X-ray sources. Here we present a novel mission, the New Hard X-ray Mission (NHXM) that brings together for the first time simultaneous high-sensitivity, hard-X-ray imaging, broadband spectroscopy and polarimetry. NHXM will…

Black-holesAcceleration mechanismCosmic Visionmedia_common.quotation_subjectPolarimetry7. Clean energy01 natural sciencesMissionsCosmologyPhysical cosmologyNon-thermal emissionAcceleration mechanism; Accretion physics; Black-holes; Compact objects; Cosmology; Missions; Non-thermal emission; X-ray imaging; X-ray polarimetry; Astronomy and Astrophysics; Space and Planetary ScienceObservatory0103 physical sciencesBroadbandX-ray polarimetry010303 astronomy & astrophysicsCompact objectsmedia_commonPhysics010308 nuclear & particles physicsX-ray imagingVegaAstronomyAstronomy and AstrophysicsAccretion physicsCosmologySkySpace and Planetary ScienceExperimental Astronomy
researchProduct

Innovative Non-Thermal Technologies for Recovery and Valorization of Value-Added Products from Crustacean Processing By-Products—An Opportunity for a…

2021

The crustacean processing industry has experienced significant growth over recent decades resulting in the production of a great number of by-products. Crustacean by-products contain several valuable components such as proteins, lipids, and carotenoids, especially astaxanthin and chitin. When isolated, these valuable compounds are characterized by bioactivities such as anti-microbial, antioxidant, and anti-cancer ones, and that could be used as nutraceutical ingredients or additives in the food, pharmaceutical, and cosmetic industries. Different innovative non-thermal technologies have appeared as promising, safe, and efficient tools to recover these valuable compounds. This review aims at …

CarotenoidNon-thermal technologieHealth (social science)Circular economyChemical technologySeafood industrycarotenoidsnon-thermal technologiesPlant ScienceReviewTP1-1185ReuseHealth Professions (miscellaneous)MicrobiologyastaxanthinNutraceuticalSustainabilityvaluable compoundsBiochemical engineeringBusinessValue addedchitosanFood ScienceFoods
researchProduct

Recent advances in the application of pulsed light processing for improving food safety and increasing shelf life

2019

Abstract Background New technologies of non-thermal disinfection such as pulsed light (PL) have emerged lately as an alternative to traditional (thermal and chemical) disinfection and preservation methods. PL can be used to decontaminate a great variety of foods as well as to decontaminate contact surfaces, thus improving safety in foods and extending their shelf life. Moreover, this technology can prevent or reduce some of the detrimental effects of traditional methods on nutrients and bioactive compounds of food products. Scope and approach The combination of PL with other techniques such as ultraviolet light (UV), thermosonication (TS), pulsed electric fields (PEF), manothermosonication …

Nutritive value0303 health sciencesPreservation methods030306 microbiologybusiness.industry04 agricultural and veterinary sciencesHuman decontaminationContaminationShelf lifeFood safety040401 food scienceMicrobial inactivation03 medical and health sciences0404 agricultural biotechnologyContact surfacesPulsed lightSensory propertiesUltraviolet lightNon-thermal technologyEnvironmental scienceMicrobial decontaminationbusinessProcess engineeringFood ScienceBiotechnologyTrends in Food Science & Technology
researchProduct