0000000000634046

AUTHOR

Masa Lakicevic

showing 2 related works from this author

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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Dust Production and Particle Acceleration in Supernova 1987A Revealed with ALMA

2013

Supernova (SN) explosions are crucial engines driving the evolution of galaxies by shock heating gas, increasing the metallicity, creating dust, and accelerating energetic particles. In 2012 we used the Atacama Large Millimeter/Submillimeter Array to observe SN 1987A, one of the best-observed supernovae since the invention of the telescope. We present spatially resolved images at 450um, 870um, 1.4mm, and 2.8mm, an important transition wavelength range. Longer wavelength emission is dominated by synchrotron radiation from shock-accelerated particles, shorter wavelengths by emission from the largest mass of dust measured in a supernova remnant (>0.2Msun). For the first time we show unambig…

MetallicityAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSynchrotron radiationAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSubmillimeter ArrayEARLY UNIVERSEindividual (1987A) [supernovae]Magellanic CloudsAstrophysics::Solar and Stellar AstrophysicsEjectaSupernova remnantSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsQBHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsISM [galaxies]supernova remnants [ISM]Astronomy and AstrophysicsOPTICAL-PROPERTIESHUBBLE-SPACE-TELESCOPEAstrophysics - Astrophysics of GalaxiesEVOLUTIONGalaxyParticle accelerationEJECTASupernovaPhysics and AstronomyAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)REVERSE SHOCKREMNANTAstrophysics::Earth and Planetary AstrophysicsEMISSIONAstrophysics - High Energy Astrophysical PhenomenaMASSIVE STARSSN 1987A
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