Gamma-Ray Line Emission from Superbubbles

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dc.creatorParizot, Etienne
dc.creatorKnodlseder, Jurgen
dc.date1999-03-11
dc.date.accessioned2026-07-07T02:30:47Z
dc.date.available2026-07-07T02:30:47Z
dc.descriptionWe present an evolutionary model for gamma-ray line emission from superbubbles based on shock acceleration of metal-rich stellar ejecta. Application to the Orion OB1 association shows that gamma-ray lines at the detection threshold of the SPI spectrometer aboard of INTEGRAL are expected, making this region an interesting target for studies of the interaction of supernova shocks with the interstellar medium.
dc.description4 pages, 2 figures, Proc. of the 3rd INTEGRAL workshop, Taormina
dc.identifierhttps://arxiv.org/abs/astro-ph/9903170
dc.identifierhttp://arxiv.org/abs/astro-ph/9903170
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13937
dc.subjectAstrophysics
dc.titleGamma-Ray Line Emission from Superbubbles
dc.typetext

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