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                <text>Over the past 200 years, our knowledge of stars has expanded enormously. From seeing myriad dots of different brightnesses, we have moved on to measure their distances, temperatures, sizes, chemical compositions, and even ages, finding both young and ancient stars that dwarf our Sun and are dwarfed by it. Unique in its approach, Extreme Stars describes the lives of stars from a new perspective by examining their amazing features. The result is a refreshing, up-to-date, and engaging overview of stellar evolution, suitable for everyone interested in viewing or studying the stars. Ten chapters, generously illustrated throughout, explain the natures of the brightest, the largest, the hottest, and the youngest, among other kinds of stars, ending with a selection of the strangest stars the Universe has to offer. Extreme Stars shows how stars develop and die and how each extreme turns into another under the inexorable twin forces of time and gravity.</text>
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                <text>This book provides a comprehensive overview of the history of ideas about the sun and the stars, from antiquity to modern times. Two theoretical astrophysicists who have been active in the field since the early 1960s tell the story in fluent prose. About half of the book covers most of the theoretical research done from 1940 to the close of the twentieth century, a large body of work that has to date been little explored by historians.&lt;br /&gt;
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                <text>In this jargon-free review of one of the most fascinating topics in modern science, acclaimed science writer Kitty Ferguson examines the discovery of black holes, their nature, and what they can teach us about the mysteries of the universe. In search of the answers, we trace a star from its birth to its death throes, take a hypothetical journey to the border of a black hole and beyond, spend time with some of the world's leading theoretical physicists and astronomers, and take a whimsical look at some of the wild ideas black holes have inspired. Prisons of Light--Black Holes is comprehensive and detailed. Yet Kitty Ferguson's lightness of touch and down-to-earth analogies set this book apart from all others on black holes and make it a wonderfully stimulating and entertaining read.</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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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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                <text>This book is an introduction to “multi-messenger” astrophysics. It covers the many different aspects connecting particle physics with astrophysics and cosmology and introduces astrophysics using numerous experimental findings recently obtained through the study of high-energy particles.&lt;br /&gt;
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;
With his research he is involved in experimental physics, with particular interest in high-energy physics without particle accelerators and astroparticle physics.&lt;br /&gt;
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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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;
Na een korte inleiding over de Zon en haar planeten, geeft dit boek een overzicht van de waarnemingen die aan onze huidige kennis ten grondslag liggen, en van de natuurkunde die het leven van de sterren beschrijft. Vervolgens geeft het een beschrijving van geboorte, leven en einde van sterren. Het besluit met een beschrijving van waarnemingen aan neutronensterren en zwarte gaten, en hun rol in het testen van de algemene relativiteits-theorie. Opgaven stellen de lezer in staat zich te oefenen in het handig en snel afschatten van belangrijke fysische parameters van sterren.&lt;br /&gt;</text>
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