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This second edition has been updated and revised and contains contributions covering important developments in this field, and reflecting on interesting insights into classical novae. The book examines thermonuclear processes, the evolution of nova systems, nova atmospheres and winds, the evolution of dust and molecules in novae, nova remnants and observations of novae in other galaxies. It includes observations across the electromagnetic spectrum, from radio to gamma rays, and discusses some of the most important outstanding problems in classical nova research.
Stars, New --- Etoiles temporaires --- Stars, New. --- Cataclysmic variable stars. --- Cataclysmic binary stars --- Cataclysmic variables (Stars) --- Eruptive variables (Stars) --- Explosive variables (Stars) --- Double stars --- Variable stars --- New stars --- Novae --- Cataclysmic variable stars
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Efforts to uncover the explosion mechanism of core collapse supernovae and to understand all of their associated phenomena have been ongoing for nearly four decades. Despite this, our theoretical understanding of these cosmic events remains limited; two- and three-dimensional modeling of these events is in its infancy. Most of the modeling efforts over the past four decades have, by necessity, been constrained to spherical symmetry, with the first two-dimensional, albeit simplified, models appearing only during the last decade. Simulations to understand the complex interplay between the turbul
Supernovae --- Cataclysmic variable stars. --- Cataclysmic binary stars --- Cataclysmic variables (Stars) --- Eruptive variables (Stars) --- Explosive variables (Stars) --- Double stars --- Variable stars --- Supernovas --- Cataclysmic variable stars --- X-ray sources, Galactic --- Mathematical models
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This thesis is a comprehensive work that addresses many of the open questions currently being discusssed in the very-high-energy (VHE) gamma-ray community. It presents a detailed description of the MAGIC telescope together with a glimpse of the future Cherenkov Telescope Array (CTA). One section is devoted to the design, development and characterization of trigger systems for current and future imaging atmospheric Cherenkov telescopes. The book also features a state-of-the-art description of pulsar wind nebula (PWN) systems, the study of the multi-TeV spectrum of the Crab nebula, as well as the discovery of VHE gamma rays at the multiwavelength PWN 3C 58, which were sought at these wavelengths for more than twenty years. It also includes the contextualization of this discovery amongst the current population of VHE gamma-ray PWNe. Cataclysmic variable stars represent a new source of gamma ray energies, and are also addressed here. In closing, the thesis reports on the systematic search for VHE gamma-ray emissions of AE Aquarii in a multiwavelength context and the search for VHE gamma-ray variability of novae during outbursts at different wavelengths. .
Physics. --- Observations, Astronomical. --- Astronomy --- Astrophysics. --- Astrophysics and Astroparticles. --- Astronomy, Observations and Techniques. --- Observations. --- Cataclysmic variable stars. --- Gamma-Ray Observatory. --- Cataclysmic binary stars --- Cataclysmic variables (Stars) --- Eruptive variables (Stars) --- Explosive variables (Stars) --- United States. --- GRO --- Compton Observatory --- Double stars --- Variable stars --- Astronomy—Observations. --- Astronomical observations --- Observations, Astronomical --- Astronomical physics --- Cosmic physics --- Physics
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