0000000000681469

AUTHOR

Patrick Slane

0000-0002-6986-6756

showing 2 related works from this author

B-MINE, the balloon-borne microcalorimeter nuclear line explorer

2001

B-MINE is a concept for a balloon mission designed to probe the deepest regions of a supernova explosion by detecting Ti-44 emission at 68 keV with spatial and spectral resolutions that are sufficient to determine the extent and velocity distribution of the Ti-44 emitting region. The payload introduces the concept of focusing optics and microcalorimeter spectroscopy to nuclear line emission astrophysics. B-MINE has a thin, plastic foil telescope multilayered to maximize the reflectivity in a 20 keV band centered at 68 keV and a microcalorimeter array optimized for the same energy band. This combination provides a reduced background, an energy resolution of 50 eV and a 3sigma sensitivity in …

X-ray AstronomyPhysics::Instrumentation and DetectorsSupernovaAstrophysics::High Energy Astrophysical PhenomenaBallonX-ray opticsSNRlaw.inventionAstrophysicTelescopeOpticsSettore FIS/05 - Astronomia E AstrofisicaNTD GermaniumlawMicrocalorimeterBinary starEmission spectrumX-ray OpticSpectral resolutionElectrical and Electronic EngineeringSpectroscopyLine (formation)PhysicsX-ray astronomybusiness.industryCondensed Matter PhysicsSupernovaStarsgamma rayMeasuring instrumentbusinessBalloon
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Investigating the Structure of Vela X

2018

Vela X is the prototypical example of a pulsar wind nebula whose morphology and detailed structure have been affected by the interaction with the reverse shock of its host supernova remnant. The resulting complex of filamentary structure and mixed-in ejecta embedded in a nebula that is offset from the pulsar provides the best example we have of this middle-age state that characterizes a significant fraction of composite SNRs, and perhaps all of the large-diameter PWNe seen as TeV sources. Here we report on an XMM-Newton Large Project study of Vela X, supplemented by additional Chandra observations. Through broad spectral modeling as well as detailed spectral investigations of discrete emiss…

shock waveDensity gradientAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsVela01 natural sciencesPulsar wind nebulaPulsar0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010306 general physicsEjectaSupernova remnant010303 astronomy & astrophysicsacceleration of particleISM: supernova remnantAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)NebulaAstronomy and AstrophysicsAstronomy and AstrophysicISM: individual objects (Vela X)Space and Planetary ScienceAstrophysics - High Energy Astrophysical PhenomenaEquivalent width
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