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dc.contributor.authorIsern Vilaboy, Jordi
dc.contributor.authorBravo Guil, Eduardo
dc.contributor.authorGómez, J.
dc.contributor.authorGarcía Senz, Domingo
dc.contributor.authorJean, Pierre
dc.contributor.otherUniversitat Politècnica de Catalunya. Departament de Física i Enginyeria Nuclear
dc.date.accessioned2013-07-15T08:25:16Z
dc.date.created1999-12
dc.date.issued1999-12
dc.identifier.citationIsern, J. [et al.]. Gamma-ray spectrum of type Ia supernovae. "Astrophysical letters and communications", Desembre 1999, vol. 38, núm. 1-6, p. 411-414.
dc.identifier.issn0888-6512
dc.identifier.urihttp://hdl.handle.net/2117/19950
dc.description.abstractThe explosion mechanism associated with thermonuclear supernovae (SNia) is still a matter of debate. In this paper we examine the 'f-ray emission of the radioactive debris predicted by the different theoretícal models and, using response estimations of the SPI and IBIS instruments aboard of INTEGRAL, we evaluate the capabilities of such instruments in the study of SNia. We also discuss preliminary results obtained with 3D models.
dc.format.extent4 p.
dc.language.isoeng
dc.subjectÀrees temàtiques de la UPC::Física::Astronomia i astrofísica
dc.subject.lcshSupernovae
dc.subject.otherSupernovae
dc.subject.otherGamma-rays
dc.titleGamma-ray spectrum of type Ia supernovae
dc.typeArticle
dc.subject.lemacSupernoves
dc.contributor.groupUniversitat Politècnica de Catalunya. GAA - Grup d'Astronomia i Astrofísica
dc.rights.accessRestricted access - publisher's policy
local.identifier.drac1222176
dc.description.versionPostprint (published version)
dc.date.lift10000-01-01
local.citation.authorIsern, J.; Bravo, E.; Gómez, J.; Garcia, D.; Jean, P.
local.citation.publicationNameAstrophysical letters and communications
local.citation.volume38
local.citation.number1-6
local.citation.startingPage411
local.citation.endingPage414


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