0000000000965663

AUTHOR

Christopher Stockdale

showing 2 related works from this author

A decade of SN 1993J : discovery of radio wavelength effects in the expansion rate

2009

We studied the growth of the shell-like radio structure of supernova SN 1993J in M 81 from September 1993 to October 2003 with very-long-baseline interferometry (VLBI) observations at the wavelengths of 3.6, 6, and 18 cm. We developed a method to accurately determine the outer radius (R) of any circularly symmetric compact radio structure such as SN 1993J. The source structure of SN 1993J remains circularly symmetric (with deviations from circularity under 2%) over almost 4000 days. We characterize the decelerated expansion of SN 1993J until approximately day 1500 after explosion with an expansion parameter m = 0.845 ± 0.005 (R ∝ tm). However, from that day onwards the expansion differs whe…

PhysicsOpacitygeneral [Supernovae]Astronomy and AstrophysicsRadiusAstrophysics:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Galaxias [UNESCO]clusters : individual : M 81 [Galaxies]Magnetic fieldInterpretation (model theory)SupernovaWavelengthGalaxies : clusters : individual : M 81; Radio continuum : stars; Supernovae : general; Supernovae : individual : SN 1993J; Techniques : interferometricSpace and Planetary ScienceVery-long-baseline interferometryinterferometric [Techniques]stars [Radio continuum]UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Estrellasindividual : SN 1993J [Supernovae]EjectaUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Galaxias:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Estrellas [UNESCO]
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8.4GHz VLBI observations of SN2004et in NGC6946

2007

We report on 8.4GHz Very Long Baseline Interferometry (VLBI) observations of the type II-P supernova SN2004et in the spiral galaxy NGC 6946, made on 20 February 2005 (151 days after explosion). The Very Large Array (VLA) flux density was 1.23$\pm$0.07 mJy, corresponding to an isotropic luminosity at 8.4GHz of (4.45$\pm$0.3)$\times10^{25}$ erg s$^{-1}$ Hz$^{-1}$ and a brightness temperature of (1.3$\pm$0.3)$\times10^{8}$ K. We also provide an improved source position, accurate to about 0.5 mas in each coordinate. The VLBI image shows a clear asymmetry. From model fitting of the size of the radio emission, we estimate a minimum expansion velocity of 15,700$\pm$2,000 km s$^{-1}$. This velocity…

media_common.quotation_subjectFOS: Physical sciencesIndividualAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsAsymmetryLuminositylaw.inventionlawVery-long-baseline interferometryNGC 6946media_commonPhysicsSpiral galaxyImage (category theory)Astrophysics (astro-ph)Astronomy and AstrophysicsGalaxiesStars:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]SynchrotronSupernovaRadio continuumSupernovaeSpace and Planetary ScienceBrightness temperatureGalaxies ; Individual ; NGC 6946 ; Radio continuum ; Stars ; Supernovae ; SN 2004etUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaSN 2004et:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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