Gamma-ray diagnostics of Type Ia supernovae Predictions of observables from three-dimensional modeling

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dc.contributor.authorSumma, A
dc.contributor.authorUlyanov, A
dc.contributor.authorKromer, M
dc.contributor.authorBoyer, S
dc.contributor.authorRopke, Friedrich
dc.contributor.authorSim, Stuart A
dc.contributor.authorSeitenzahl, Ivo
dc.contributor.authorFink, M
dc.contributor.authorMannheim, K
dc.contributor.authorPakmor, R
dc.contributor.authorCiaraldi-Schoolmann, F
dc.contributor.authorDiehl, R
dc.contributor.authorMaeda, Keiichi
dc.contributor.authorHillebrandt, Wolfgang
dc.date.accessioned2018-11-29T22:52:08Z
dc.date.available2018-11-29T22:52:08Z
dc.date.issued2013
dc.date.updated2018-11-29T07:43:56Z
dc.description.abstractAlthough the question of progenitor systems and detailed explosion mechanisms still remains a matter of discussion, it is commonly believed that Type Ia supernovae (SNe Ia) are production sites of large amounts of radioactive nuclei. Even though the gamma-ray emission due to radioactive decays is responsible for powering the light curves of SNe Ia, gamma rays themselves are of particular interest as a diagnostic tool because they directly lead to deeper insight into the nucleosynthesis and the kinematics of these explosion events.
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/152091
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.subjectKeywords: Gamma rays: generals; Gamma-ray diagnostics; Line: formation; Nuclear reactions , nucleosynthesis , abundances; Radiative transfer simulations; Space observatories; Supernovae: general; Three-dimensional modeling; Chemical elements; Explosions; Gamma rays Gamma rays: general; Hydrodynamics; Line: formation; Nuclear reactions, nucleosynthesis, abundances; Radiative transfer; Supernovae: general
dc.titleGamma-ray diagnostics of Type Ia supernovae Predictions of observables from three-dimensional modeling
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issueA67
local.contributor.affiliationSumma, A, Universität Würzburg
local.contributor.affiliationUlyanov, A, University College Dublin
local.contributor.affiliationKromer, M, Max Planck Institut für Astrophysik
local.contributor.affiliationBoyer, S, Universität Würzburg
local.contributor.affiliationRopke, Friedrich, Universitat Wurzburg
local.contributor.affiliationSim, Stuart A, College of Science, ANU
local.contributor.affiliationSeitenzahl, Ivo, College of Science, ANU
local.contributor.affiliationFink, M, Universitat Wurzburg
local.contributor.affiliationMannheim, K, Universität Würzburg
local.contributor.affiliationPakmor, R, Heidelberg Institute for Theoretical Studies
local.contributor.affiliationCiaraldi-Schoolmann, F, Max-Planck-Institut für Astrophysik
local.contributor.affiliationDiehl, R, Max-Planck-Institut für extraterrestrische Physik
local.contributor.affiliationMaeda, Keiichi, University of Tokyo
local.contributor.affiliationHillebrandt, Wolfgang, Max Planck Institute for Astrophysics
local.contributor.authoremailu4967042@anu.edu.au
local.contributor.authoruidSim, Stuart A, u4967042
local.contributor.authoruidSeitenzahl, Ivo, u5472295
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
local.identifier.ariespublicationu4571891xPUB61
local.identifier.citationvolume554
local.identifier.doi10.1051/0004-6361/201220972
local.identifier.scopusID2-s2.0-84878884906
local.identifier.thomsonID000320444200066
local.identifier.uidSubmittedByu4571891
local.type.statusPublished Version

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