Results 201 to 210 of about 6,421 (225)

Type Ia Supernovae

open access: yesEAS Publications Series, 2008
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
openaire   +2 more sources

- Type Ia Supernovae

open access: yes, 2016
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
core   +4 more sources

Abundance Tomography of Type Ia Supernovae [PDF]

open access: yes, 2004
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.
openaire   +3 more sources

Multiple images of a type Ia supernova

Science, 2017
Supernovae 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
openaire   +2 more sources

Type Ia supernovae

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.
openaire   +1 more source

Gamma-ray burst jets in supernovae

New Astronomy Reviews, 2021
A Corsi, Davide Lazzati
exaly  

Peculiar-velocity cosmology with Types Ia and II supernovae

Monthly Notices of the Royal Astronomical Society, 2021
Benjamin E Stahl   +2 more
exaly  

Synthetic observables for electron-capture supernovae and low-mass core collapse supernovae

Monthly Notices of the Royal Astronomical Society, 2021
Alexandra Kozyreva   +2 more
exaly  

A generalized semi-analytic model for magnetar-driven supernovae

Monthly Notices of the Royal Astronomical Society, 2023
Conor M B Omand   +2 more
exaly  

Low luminosity Type II supernovae – IV. SN 2020cxd and SN 2021aai, at the edges of the sub-luminous supernovae class

Monthly Notices of the Royal Astronomical Society, 2022
G Valerin, M L Pumo, A Pastorello
exaly  

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