Search results for "SN-1987A"

showing 2 items of 2 documents

Carbon Monoxide in the Cold Debris of Supernova 1987A

2013

We report spectroscopic and imaging observations of rotational transitions of cold CO and SiO in the ejecta of SN1987A, the first such emission detected in a supernova remnant. In addition to line luminosities for the CO J=1-0, 2-1, 6-5, and 7-6 transitions, we present upper limits for all other transitions up to J=13-12, collectively measured from the Atacama Large Millimeter Array (ALMA), the Atacama Pathfinder EXperiment (APEX), and the Herschel Spectral and Photometric Imaging REceiver (SPIRE). Simple models show the lines are emitted from at least 0.01 solar masses of CO at a temperature > 14 K, confined within at most 35% of a spherical volume expanding at ~ 2000 km/s. Moreover, we…

FOS: Physical sciencesAstrophysicsWAVELENGTHindividual (SN1987A) [supernovae]FACILITYEjectaSupernova remnantSolar and Stellar Astrophysics (astro-ph.SR)3-DIMENSIONAL STRUCTURELine (formation)PhysicsSolar massSN-1987AINSTRUMENTsupernova remnants [ISM]Astronomy and AstrophysicsAtacama Large Millimeter ArrayDebrisSupernovaSpireEJECTACASSIOPEIAPhysics and AstronomyAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceREMNANTSN 1987A
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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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