Gamma-ray spectrum of type Ia supernovae
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Document typeArticle
Defense date1999-12
Rights accessRestricted access - publisher's policy
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Abstract
The 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.
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.
ISSN0888-6512
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