Search results for "PARTICLE-ACCELERATION"

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Spectral and morphological analysis of the remnant of Supernova 1987A with ALMA and ATCA

2014

We present a comprehensive spectral and morphological analysis of the remnant of Supernova (SN) 1987A with the Australia Telescope Compact Array (ATCA) and the Atacama Large Millimeter/submillimeter Array (ALMA). The non-thermal and thermal components of the radio emission are investigated in images from 94 to 672 GHz ($\lambda$ 3.2 mm to 450 $\mu$m), with the assistance of a high-resolution 44 GHz synchrotron template from the ATCA, and a dust template from ALMA observations at 672 GHz. An analysis of the emission distribution over the equatorial ring in images from 44 to 345 GHz highlights a gradual decrease of the east-to-west asymmetry ratio with frequency. We attribute this to the shor…

PARTICLE-ACCELERATIONAstrophysics::High Energy Astrophysical PhenomenaLIGHT-CURVEAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsPulsar wind nebulaSubmillimeter ArrayGALACTIC RADIO EMISSIONlaw.inventionneutron [stars]Far infraredPulsarlawQCAstrophysics::Galaxy AstrophysicsQBPhysicsSN-1987ANEUTRINO BURSTsupernova remnants [ISM]RAY-EMISSIONMAGNETIC-FIELDAstronomy and AstrophysicsPULSARnon-thermal [radiation mechanisms]SynchrotronEVOLUTIONSupernovaPhysics and Astronomyindividual (SN 1987A) [supernovae]Space and Planetary Sciencethermal [radiation mechanisms]Spectral energy distributiongeneral [radio continuum]MillimeterAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaSN 1987A
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The cosmic ray proton plus helium energy spectrum measured by the ARGO-YBJ experiment in the energy range 3-300 TeV

2015

The ARGO-YBJ experiment is a full-coverage air shower detector located at the Yangbajing Cosmic Ray Observatory (Tibet, People's Republic of China, 4300 m a.s.l.). The high altitude, combined with the full-coverage technique, allows the detection of extensive air showers in a wide energy range and offer the possibility of measuring the cosmic ray proton plus helium spectrum down to the TeV region, where direct balloon/space-borne measurements are available. The detector has been in stable data taking in its full configuration from November 2007 to February 2013. In this paper the measurement of the cosmic ray proton plus helium energy spectrum is presented in the region 3-300 TeV by analyzi…

Nuclear and High Energy PhysicsPARTICLE-ACCELERATIONPhysics and Astronomy (miscellaneous)ProtonAstrophysics::High Energy Astrophysical PhenomenaSHELLFOS: Physical sciencesCosmic rayAstrophysics01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Observatory0103 physical sciencesUltra-high-energy cosmic ray010306 general physicsCosmic-ray observatoryDETECTORNuclear and High Energy PhysicPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)AIR-SHOWERSSpectral index010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsSpectral densityAir shower13. Climate actionSUPERNOVA REMNANTHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical Phenomena
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