Search results for "jets [Galaxies]"

showing 10 items of 488 documents

X-ray emission from stellar jets by collision against high-density molecular clouds: an application to HH 248

2015

We investigate the plausibility of detecting X-ray emission from a stellar jet that impacts against a dense molecular cloud. This scenario may be usual for classical T Tauri stars with jets in dense star-forming complexes. We first model the impact of a jet against a dense cloud by 2D axisymmetric hydrodynamic simulations, exploring different configurations of the ambient environment. Then, we compare our results with XMM-Newton observations of the Herbig-Haro object HH 248, where extended X-ray emission aligned with the optical knots is detected at the edge of the nearby IC 434 cloud. Our simulations show that a jet can produce plasma with temperatures up to 10 MK, consistent with producti…

AstrofísicaHERBIGHARO OBJECTSJETS AND OUTFLOWS [ISM]Astrophysics::High Energy Astrophysical PhenomenaRotational symmetryFOS: Physical sciencesCloud computingAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsISM [X-RAYS]Space (mathematics)LuminosityHYDRODYNAMICS//purl.org/becyt/ford/1 [https]INDIVIDUAL OBJECTS (HH 248) [ISM]hydrodynamics Herbig-Haro objects ISM: individual objects: HH 248 ISM: jets and outflows X-rays: ISMAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)PhysicsJet (fluid)business.industryMolecular cloudAstronomy and Astrophysics//purl.org/becyt/ford/1.3 [https]PlasmaAstronomíaT Tauri starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceHerbig–Haro objectsbusiness
researchProduct

Formation of X-ray emitting stationary shocks in magnetized protostellar jets

2016

X-ray observations of protostellar jets show evidence of strong shocks heating the plasma up to temperatures of a few million degrees. In some cases, the shocked features appear to be stationary. They are interpreted as shock diamonds. We aim at investigating the physics that guides the formation of X-ray emitting stationary shocks in protostellar jets, the role of the magnetic field in determining the location, stability, and detectability in X-rays of these shocks, and the physical properties of the shocked plasma. We performed a set of 2.5-dimensional magnetohydrodynamic numerical simulations modelling supersonic jets ramming into a magnetized medium and explored different configurations…

AstrofísicaMagnetohydrodynamics (MHD)010504 meteorology & atmospheric sciencesRadiative coolingAstrophysics::High Energy Astrophysical PhenomenaISM: structureFOS: Physical sciencesAstrophysics01 natural sciencesISM: magnetic field0103 physical sciencesShock diamondRadiative transfer010303 astronomy & astrophysicsISM: jets and outflowSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Jet (fluid)Astronomy and AstrophysicsPlasmaAstronomy and AstrophysicThermal conductionX-rays: ISMShock (mechanics)Magnetic fieldAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceStars: protostarAstrophysics - High Energy Astrophysical Phenomena
researchProduct

Stability analysis of relativistic jets from collapsars and its implications on the short-term variability of gamma-ray bursts

2002

We consider the transverse structure and stability properties of relativistic jets formed in the course of the collapse of a massive progenitor. Our numerical simulations show the presence of a strong shear in the bulk velocity of such jets. This shear can be responsible for a very rapid shear--driven instability that arises for any velocity profile. This conclusion has been confirmed both by numerical simulations and theoretical analysis. The instability leads to rapid fluctuations of the main hydrodynamical parameters (density, pressure, Lorentz factor, etc.). However, the perturbations of the density are effectively decoupled from those of the pressure because the beam of the jet is radi…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesgalaxies jetsAstrophysicsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAInstabilitysymbols.namesakeAstrophysical jetISM jets and outflowsPhysicsBurstsGamma ray theoryTurbulenceAstrophysics (astro-ph)Magnetohydradynamics (MHD) : Gamma rays ; Bursts ; Gamma ray theory ; ISM jets and outflows ; galaxies jetsAstronomy and AstrophysicsMechanicsLight curve:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Transverse planeLorentz factorSpace and Planetary SciencesymbolsGamma rays [Magnetohydradynamics (MHD)]OutflowUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaGamma-ray burst:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
researchProduct

"Table 11" of "Searches for supersymmetry with the ATLAS detector using final states with two leptons and missing transverse momentum in sqrt{s} = 7 …

2011

The missing-mass ET distribution for opposite-sign dilepton events before any jet requirement.

Astrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyNuclear TheorySUSY7000.0Single Differential DistributionJet ProductionInclusiveProton-Proton ScatteringP P --> LEPTON+ LEPTON- JETS XDN/DETHigh Energy Physics::ExperimentSupersymmetryNuclear ExperimentDrell Yan
researchProduct

On the nature of the soft γ-ray emission in the hard state of the black hole transient GRS 1716-249

2020

The black hole transient GRS 1716-249 was monitored from the radio to the gamma-ray band during its 2016-2017 outburst. This paper focuses on the Spectral Energy Distribution (SED) obtained in 2017 February-March, when GRS 1716-249 was in a bright hard spectral state. The soft gamma-ray data collected with the INTEGRAL/SPI telescope show the presence of a spectral component which is in excess of the thermal Comptonisation emission. This component is usually interpreted as inverse Compton emission from a tiny fraction of non-thermal electrons in the X-ray corona. We find that hybrid thermal/non-thermal Comptonisation models provide a good fit to the X/gamma-ray spectrum of GRS 1716-249. The …

Astrophysics::High Energy Astrophysical Phenomenablack hole physicsFOS: Physical sciencesElectronAstrophysics7. Clean energy01 natural sciencesSpectral lineX-rays: binariesaccretion0103 physical sciences010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)Accretion (meteorology)010308 nuclear & particles physicsAstronomy and Astrophysicsgamma-rays: generalSpectral componentaccretion discsCoronaBlack holeISM: jets and outflowsSpace and Planetary ScienceSpectral energy distributionAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
researchProduct

M'as-tu vu ?

2022

Chaussures -- AntiquitéParfums -- AntiquitéAccessoire du costumeépilationObjets de toiletteAccessoire du vêtementPortraits officielsMaquillage -- AntiquitéCatalogue d'expositionCosmétiques -- AntiquitéMarqueur socialPratiques balnéairesApparenceSoins du corpsCoiffurePratiques d'hygièneAmulettesBeauté -- AntiquitéThermes romainsStatut social -- Antiquité[SHS.ARCHEO] Humanities and Social Sciences/Archaeology and PrehistorySaletéPilositéPropretéNormes sociales -- AntiquitéSanté -- AntiquitéTombe à hypogéeAttributs d’apparenceObjets archéologiquesFibulesStèles funérairesNécropole gallo-romaineParure[SHS] Humanities and Social SciencesVêtements -- Antiquité
researchProduct

"Table 3" of "Search for supersymmetry using final states with one lepton, jets, and missing transverse momentum with the ATLAS detector in sqrt{s} =…

2011

Distribution of M(C=EFFECTIVE) IN GEV for data and background MC calculation.

Computer Science::Software EngineeringSUSY7000.0Jet ProductionNInclusiveProton-Proton ScatteringComputer Science::Programming LanguagesCondensed Matter::Strongly Correlated ElectronsHigh Energy Physics::ExperimentP P --> LEPTON+ JETS XP P --> LEPTON- JETS XSupersymmetryNuclear Experiment
researchProduct

"Table 23" of "Studies of W boson plus jets production in p\bar{p} collisions at sqrt(s)=1.96 TeV"

2013

Differential production cross-section, normalized to the measured inclusive W boson cross-section, as a function of W boson pT for events with two or more jets produced in association with a W boson. First uncertainty is statistical, second uncertainty is systematic.

Condensed Matter::Quantum GasesDijet ProductionInclusiveSingle Differential Cross SectionHigh Energy Physics::PhenomenologyPBAR P --> W+ JETS XPBAR P --> W- JETS XDSIG/DPTJet ProductionTransverse Momentum Dependence1960.0W Production
researchProduct

"Table 2" of "Determination of A(b)(FB) using jet charge measurements in Z decays."

1998

The combination of the data on and off peak of Z-boson.

Condensed Matter::Quantum GasesE+ E- --> BQ BQBARInclusiveAsymmetry MeasurementE+ E- --> Z0E+ E- ScatteringHigh Energy Physics::PhenomenologyExclusiveJet ProductionE+ E- --> JETS XASYM91.0
researchProduct

"Table 3" of "Determination of A(b)(FB) using jet charge measurements in Z decays."

1998

The combination of the data on and off peak of Z-boson.

Condensed Matter::Quantum GasesE+ E- --> BQ BQBARInclusiveSIN2TWE+ E- --> Z0E+ E- ScatteringHigh Energy Physics::PhenomenologyExclusiveJet ProductionE+ E- --> JETS X91.0
researchProduct