0000000000625311

AUTHOR

Jacco Th. Van Loon

showing 2 related works from this author

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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High Angular Resolution ALMA Images of Dust and Molecules in the SN 1987A Ejecta

2019

We present high angular resolution (~80 mas) ALMA continuum images of the SN 1987A system, together with CO $J$=2 $\!\rightarrow\!$ 1, $J$=6 $\!\rightarrow\!$ 5, and SiO $J$=5 $\!\rightarrow\!$ 4 to $J$=7 $\!\rightarrow\!$ 6 images, which clearly resolve the ejecta (dust continuum and molecules) and ring (synchrotron continuum) components. Dust in the ejecta is asymmetric and clumpy, and overall the dust fills the spatial void seen in H$\alpha$ images, filling that region with material from heavier elements. The dust clumps generally fill the space where CO $J$=6 $\!\rightarrow\!$ 5 is fainter, tentatively indicating that these dust clumps and CO are locationally and chemically linked. In t…

astro-ph.SR010504 meteorology & atmospheric sciencesFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesSpectral lineNucleosynthesis0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsMoleculeEjecta010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstronomy and AstrophysicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceSpectral energy distributionAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]QB799The Astrophysical Journal
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