5.9-keV Mn K-shell X-ray luminosity from the decay of $^55$Fe in Type Ia supernova models
Seitenzahl, I.~R. and Summa, A. and Krauss, F. and Sim, S.~A. and Diehl, R. and Els_s06sser, D. and Fink, M. and Hillebrandt, W. and Kromer, M. and Ma
Keywords
line: formation, nuclear reactions, nucleosynthesis, abundances, radiative transfer, supernovae: general, white dwarfs, X-rays: general
Abstract
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