Year: 2016
Type: article
Abstract: Context. The optical light curve of Type Ia supernovae (SNIa) is powered by thermalized gamma-rays produced by the decay of 56Ni and 56Co, the main radioactive isotopes synthesized by the thermonuclear explosion of a C/O white dwarf.
Source: Astronomy and Astrophysics
Authors: J. Isern, P. Jean, E. Bravo, J. Knödlseder, F. Lebrun, E. Churazov, R. Sunyaev, A. Domingo, C. Badenes, D. H. Hartmann, P. Hoeflich, M. Renaud, S. Soldi, N. Elias-Rosa, M. Hernanz, I. Domínguez, D. García-Senz, G. G. Lichti, G. Vedrenne, P. Von Ballmoos
Institutions: Institute of Space Sciences, Université Toulouse III - Paul Sabatier, Institut de Recherche en Astrophysique et Planétologie, Université de Toulouse, Universitat Politècnica de Catalunya, Centre National de la Recherche Scientifique, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Laboratoire AstroParticule et Cosmologie, Sorbonne Paris Cité, Institut National de Physique Nucléaire et de Physique des Particules, Space Research Institute, Max Planck Institute for Astrophysics, Consejo Superior de Investigaciones Científicas, Centro de Astrobiología, University of Pittsburgh, Clemson University, Florida State University, Laboratoire Univers et Particules de Montpellier, Université Montpellier 2, Osservatorio Astronomico di Padova, National Institute for Astrophysics, Universidad de Granada, Max Planck Institute for Extraterrestrial Physics
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
Award: G6941434661
OpenAlex ID: W2254092018