Rights accessRestricted access - publisher's policy
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.
All rights reserved. This work is protected by the corresponding intellectual and industrial
property rights. Without prejudice to any existing legal exemptions, reproduction, distribution, public
communication or transformation of this work are prohibited without permission of the copyright holder