Results 151 to 160 of about 823 (184)
Stability of asymmetric Schwarzschild-Rindler-de Sitter thin shell wormhole. [PDF]
Sci RepEid A, Alkaoud A, Khader MM, Bakry MA.
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Time-Delay Cosmography: Measuring the Hubble Constant and Other Cosmological Parameters with Strong Gravitational Lensing. [PDF]
Space Sci RevBirrer S +8 more
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Primitive asteroids as a major source of terrestrial volatiles. [PDF]
Sci AdvMartins R +5 more
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Overview of the ESCAPE Dark Matter Test Science Project for astronomers. [PDF]
Open Res EurPearson J +3 more
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Curvature estimation techniques for advancing neurodegenerative disease analysis: a systematic review of machine learning and deep learning approaches. [PDF]
Am J Neurodegener DisSadegh-Zadeh SA +5 more
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EAS 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
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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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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.
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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.
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New Astronomy Reviews, 2010
Abstract Recent progress in modeling type Ia supernovae by means of three-dimensional hydrodynamic simulations as well as several of the still open questions are addressed in this article. It will be shown that the new models have considerable predictive power which allows us to study observable properties such as light curves and spectra without ...
Hillebrandt, W., Röpke, F.
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Abstract Recent progress in modeling type Ia supernovae by means of three-dimensional hydrodynamic simulations as well as several of the still open questions are addressed in this article. It will be shown that the new models have considerable predictive power which allows us to study observable properties such as light curves and spectra without ...
Hillebrandt, W., Röpke, F.
openaire +2 more sources