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                <text>The physics of stars</text>
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                <text>A compact yet comprehensive account concerned with how key aspects of stellar structure, evolution and nucleosynthesis can be understood in terms of basic physics. Begins with the most elementary factors and progresses to more advanced physical concepts. The author has been careful not to avoid more complex issues, instead carefully explaining each topic before it is applied. Provides a balanced treatment of fundamental physics and astrophysics and the relationship between them. Features an abundance of theoretical models, questions and hints for solution.</text>
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                <text>This textbook gives a clear account of the manner in which knowledge in many branches of physics such as gravitation, thermodynamics, atomic physics and nuclear physics can be combined to gain an understanding of the structure and evolution of stars. A major aim is to present the subject as one in which advances are still being made. The first half is an account of the observational properties of stars and a discussion of the equations that govern their structure. The second part discusses recent theoretical work on stellar evolution. The successes of the theory are stressed, but attention is also drawn to phenomena that are not completely understood.</text>
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                <text>How does it happen that billions of stars can cooperate to produce the beautiful spirals that characterize so many galaxies, including ours? This book reviews the history behind the discovery of spiral galaxies and the problems faced when trying to explain the existence of spiral structure within them. In the book, subjects such as galaxy morphology and structure are addressed as well as several models for spiral structure. The evidence in favor or against these models is discussed. The book ends by discussing how spiral structure can be used as a proxy for other properties of spiral galaxies, such as their dark matter content and their central supermassive black hole masses, and why this is important.</text>
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                <text>On July 23, 1999, the Chandra X-Ray Observatory, the most powerful X-ray telescope ever built, was launched aboard the space shuttle Columbia. Since then, Chandra has given us a view of the universe that is largely hidden from telescopes sensitive only to visible light. In Chandra's Cosmos, the Smithsonian Astrophysical Observatory's Chandra science spokesperson Wallace H. Tucker uses a series of short, connected stories to describe the telescope's exploration of the hot, high-energy face of the universe. The book is organized in three parts: "The Big," covering the cosmic web, dark energy, dark matter, and massive clusters of galaxies; "The Bad," exploring neutron stars, stellar black holes, and supermassive black holes; and "The Beautiful," discussing stars, exoplanets, and life.&lt;br /&gt;&lt;br /&gt;
Chandra has imaged the spectacular, glowing remains of exploded stars and taken spectra showing the dispersal of their elements. Chandra has observed the region around the supermassive black hole in the center of our Milky Way and traced the separation of dark matter from normal matter in the collision of galaxies, contributing to both dark matter and dark energy studies. Tucker explores the implications of these observations in an entertaining, informative narrative aimed at space buffs and general readers alike.</text>
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                <text>Compiled by a team of experts, this textbook introduces the properties and evolution of the most immediately visible objects in the Universe – stars. Designed for elementary university courses in astronomy and astrophysics, it starts with a detailed discussion of our nearest star, the Sun, and describes how solar physicists have come to understand its internal workings. It then considers how we study the basic physical properties and life-cycles of more distant stars, culminating with a discussion of more 'exotic' objects, such as neutron stars and black holes. This second edition has a greater emphasis on the physical and spectral properties of stars, introducing stellar atmospheres, spectral line formation and the role of binary stars in the formation of compact objects. Avoiding complex mathematics, and generously illustrated in colour throughout, this accessible text is ideal for self-study and will appeal to both amateur astronomers and undergraduate students.&lt;br /&gt;&lt;br /&gt;
Written by a team of experts in an accessible style that avoids complex mathematics, and illustrated in colour throughout&lt;br /&gt;&lt;br /&gt;
Contains numerous pedagogical features including boxed summaries, brief biographies of pioneering astronomers, bulleted questions and answers throughout, over 100 exercises with full solutions, and a glossary of terms&lt;br /&gt;&lt;br /&gt;
Fully updated to include recent observations and space mission results and to reflect current understanding&lt;br /&gt;</text>
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Taking a systematic approach, it comprehensively presents experimental aspects from the most advanced laboratories and detectors, as well as the theoretical background. The book is aimed at graduate students and post-graduate researchers with a basic understanding of particle and nuclear physics. It will also be of interest to particle physicists working in accelerator/collider physics who are keen to understand the mechanisms of the largest accelerators in the Universe.&lt;br /&gt;&lt;br /&gt;
The book draws on the extensive lecturing experience of Professor Maurizio Spurio from the University of Bologna.&lt;br /&gt;&lt;br /&gt;
Maurizio Spurio is a Professor of Physics at the University of Bologna where he teaches Particle and Astroparticle physics.&lt;br /&gt;
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He was member of the MACRO experiment at Gran Sasso underground laboratory, which provided a deep study of the penetrating component of the cosmic radiation including the observation of atmospheric neutrino oscillations. Since 2001 he is member of the ANTARES experiment (the first neutrino telescope in the sea), currently in charge as deputy spokesperson.&lt;br /&gt;
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                <text> &lt;br /&gt;&lt;br /&gt;
Inhoud In de laatste jaren van de 20e eeuw is onze kennis over sterren en planetenstelsels enorm toegenomen door de grotere nauwkeurigheid van technologisch ernieuwde telescopen. Dat leverde veel nieuwe ontdekkingen op, zoals de neutrino's van de Zon, trans-neptuniaanse planeten, bruine dwergen, neutronensterren en zwarte gaten.&lt;br /&gt;&lt;br /&gt;
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                <text>Introduces the physics behind single and binary stellar evolution, assuming no prior knowledge of astronomy 
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Vakgroep Fysica en Sterrenkunde&lt;br /&gt;&lt;br /&gt;&lt;br /&gt;
Datareductie en stabiliteitsanalyse van IC3328&lt;br /&gt;&lt;br /&gt;
Masterproef ingediend tot het behalen van de graad&lt;br /&gt;
Master in de Fysica en Sterrenkunde&lt;br /&gt;&lt;br /&gt;&lt;br /&gt;</text>
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                <text>From supernovae and gamma-ray bursts to the accelerating Universe, this is an exploration of the intellectual threads that lead to some of the most exciting ideas in modern astrophysics and cosmology. This fully updated second edition incorporates new material on binary stars, black holes, gamma-ray bursts, worm-holes, quantum gravity and string theory. It covers the origins of stars and their evolution, the mechanisms responsible for supernovae, and their progeny, neutron stars and black holes. It examines the theoretical ideas behind black holes and their manifestation in observational astronomy and presents neutron stars in all their variety known today. This book also covers the physics of the twentieth century, discussing quantum theory and Einstein's gravity, how these two theories collide, and the prospects for their reconciliation in the twenty-first century. This will be essential reading for undergraduate students in astronomy and astrophysics, and an excellent, accessible introduction for a wider audience.&lt;br /&gt;&lt;br /&gt;&lt;br /&gt;</text>
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