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.
- Title
- Gamma-Ray emission from SN2014J near maximum optical light
- Creators - without role
- J. Isern - Institute of Space SciencesP. Jean - Université Toulouse III - Paul SabatierE. Bravo - Universitat Politècnica de CatalunyaJürgen Knödlseder - Université Toulouse III - Paul SabatierF. Lebrun - Sorbonne Paris CitéE. Churazov - Space Research InstituteR. Sunyaev - Space Research InstituteA. Domingo - Centro de AstrobiologíaC. Badenes - University of PittsburghD.H. Hartmann - Clemson UniversityP. Hoeflich - Florida State UniversityMatthieu Renaud - Université de Montpellier, Laboratoire Univers et Particules de Montpellier - LUPMS. Soldi - Centre National de la Recherche ScientifiqueN. Elias-Rosa - Osservatorio Astronomico di PadovaM. Hernanz - Institute of Space SciencesI. DomínguezD. García-SenzG.G. Lichti - Max Planck Institute for Extraterrestrial PhysicsG. Vedrenne - Université Toulouse III - Paul SabatierP. von Ballmoos - Roche
- Publication Details
- Astronomy & Astrophysics - A&A, Vol.588
- Identifiers
- 9939425209311
- Academic Unit
- Laboratoire Univers et Particules de Montpellier - LUPM
- Language
- English
- Resource Type
- Journal article
- Local Fields
- hal-01554942