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Type Ia supernovae are thought to be the outcome of the thermonuclear explosion of a carbon–oxygen white dwarf in a close binary system. In this review we discuss the observational background, the possible progenitors, the mechanisms leading to the instability and the development of the explosion itself as well as the remaining uncertainties.
J. Isern, E. Bravo, A. Hirschmann
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Type Ia supernovae play an important role in many areas of astrophysics, as extragalactic distance indicators and the most mature probes of cosmic acceleration, as the main producers of iron in the Universe, as end points of stellar evolution, and as contributors to the chemical evolution of galaxies.
Maguire, Kate, Kate Maguire
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Abundance Tomography of Type Ia Supernovae [PDF]
Many uncertainties about the physics of Type Ia Supernovae have been revealed in the recent past, and numerous pieces are puzzled together to achieve a complete description of the phenomenon of thermonuclear explosions in the sky. However, very important parts are still missing.
Stehle, Matthias, Stehle, M.
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Multiple images of a type Ia supernova
Science, 2017Supernovae General relativity indicates that any sufficiently massive object bends the path of light passing by it. This effect is known as gravitational lensing. Goobar et al. have identified a supernova that is strongly lensed by a foreground galaxy, causing it to be highly magnified and splitting the light into four separate images. What is more, it
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2015
Type Ia supernovae (SNe Ia) are important cosmological probes, but we are uncertain how they explode. There are two progenitor channels for SNe~Ia: single and double degenerate white dwarf (WD) systems. In either model, we expect the system to be detectable as a Supersoft X-ray Source (SSS) for a significant amount of time before the explosion.
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Type Ia supernovae (SNe Ia) are important cosmological probes, but we are uncertain how they explode. There are two progenitor channels for SNe~Ia: single and double degenerate white dwarf (WD) systems. In either model, we expect the system to be detectable as a Supersoft X-ray Source (SSS) for a significant amount of time before the explosion.
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Peculiar-velocity cosmology with Types Ia and II supernovae
Monthly Notices of the Royal Astronomical Society, 2021Benjamin E Stahl +2 more
exaly
Synthetic observables for electron-capture supernovae and low-mass core collapse supernovae
Monthly Notices of the Royal Astronomical Society, 2021Alexandra Kozyreva +2 more
exaly
A generalized semi-analytic model for magnetar-driven supernovae
Monthly Notices of the Royal Astronomical Society, 2023Conor M B Omand +2 more
exaly

