W Hillebrandt, M Kromer, FK Röpke, AJ Ruiter - Frontiers of Physics, 2013 - Springer
Motivated by the fact that calibrated light curves of Type Ia supernovae (SNe Ia) have become a major tool to determine the expansion history of the Universe, considerable …
IR Seitenzahl, F Ciaraldi-Schoolmann… - Monthly Notices of …, 2013 - academic.oup.com
We present results for a suite of 14 three-dimensional, high-resolution hydrodynamical simulations of delayed-detonation models of Type Ia supernova (SN Ia) explosions. This …
INTRODUCTION The nature of type Ia supernovae (SNIa)—thermonuclear explosions of white dwarf (WD) stars—is an open question in astrophysics. There is a general consensus …
JCW had long wanted to write a new monograph on supernovae. Despite an immense explosion in the literature and many review articles, there had not been one since that of …
We present 2603 spectra of 462 nearby Type Ia supernovae (SNe Ia), including 2065 previously unpublished spectra, obtained during 1993–2008 through the Center for …
R Pakmor, M Kromer, FK Röpke, SA Sim, AJ Ruiter… - Nature, 2010 - nature.com
Type Ia supernovae are thought to result from thermonuclear explosions of carbon–oxygen white dwarf stars. Existing models generally explain the observed properties, with the …
The first γ-ray line originating from outside the Solar System that was ever detected is the 511 keV emission from positron annihilation in the Galaxy. Despite 30 years of intense …
D Kasen, FK Röpke, SE Woosley - Nature, 2009 - nature.com
Type Ia supernovae result when carbon-oxygen white dwarfs in binary systems accrete mass from companion stars, reach a critical mass and explode. The near uniformity of their …
C Kobayashi, SC Leung, K Nomoto - The Astrophysical Journal, 2020 - iopscience.iop.org
In our quest to identify the progenitors of Type Ia supernovae (SNe Ia), we first update the nucleosynthesis yields for both near-Chandrasekhar-(Ch) and sub-Ch-mass white dwarfs …