Results 191 to 200 of about 7,025,957 (218)
Re-recognized universality of Kozai oscillation on three-body dynamics. [PDF]
Iye M, Ito T.
europepmc +1 more source
Perspectives on the physics of late-type stars from beyond low earth orbit, the moon and mars. [PDF]
Mathur S, Santos ÂRG.
europepmc +1 more source
Physical mechanism of core-collapse supernovae that neutrinos drive. [PDF]
Yamada S +8 more
europepmc +1 more source
Stability of asymmetric Schwarzschild-Rindler-de Sitter thin shell wormhole. [PDF]
Eid A, Alkaoud A, Khader MM, Bakry MA.
europepmc +1 more source
On the progenitors of Type Ia supernovae [PDF]
We review all the models proposed for the progenitor systems of Type Ia supernovae and discuss the strengths and weaknesses of each scenario when confronted with observations. We show that all scenarios encounter at least a few serious diffculties, if taken to represent a comprehensive model for the progenitors of all Type Ia supernovae (SNe Ia ...
Paolo Mazzali
exaly +7 more sources
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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.
openaire +1 more source
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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A generalized semi-analytic model for magnetar-driven supernovae
Monthly Notices of the Royal Astronomical Society, 2023Conor Omand, Nikhil Sarin
exaly

