This textbook provides a comprehensive and lucid modern introduction to galaxies for advanced undergraduate students in astronomy and physics. Basic astrophysics, multiwavelength observations and theoretical concepts are carefully combined to develop an integrated understanding. All the necessary background astronomy is included and mathematics has been kept to the minimum required to enable the student to quickly grasp the essence of a calculation, or the basis for a method. The clear and friendly style of the text, thorough coverage of fundamentals, extensive use of up-to-date observations, and helpful problems make this an ideal introduction to galaxies and thorough preparation for more advanced texts and the research literature.
This extensively illustrated book presents the astrophysics of galaxies since their beginnings in the early Universe. It has been thoroughly revised to take into account the most recent observational data, and recent discoveries such as dark energy. There are new sections on galaxy clusters, gamma ray bursts and supermassive black holes. The authors explore the basic properties of stars and the Milky Way before working out towards nearby galaxies and the distant Universe. They discuss the structures of galaxies and how galaxies have developed, and relate this to the evolution of the Universe. The book also examines ways of observing galaxies across the whole electromagnetic spectrum, and explores dark matter and its gravitational pull on matter and light. This book is self-contained and includes several homework problems with hints. It is ideal for advanced undergraduate students in astronomy and astrophysics.
In diesem kompetent geschriebenen Lehrbuch wird, ausgehend von der Beschreibung unserer Milchstraße, die Astronomie der Galaxien und ihrer großräumigen Verteilung eingehend dargestellt und schließlich im kosmologischen Kontext diskutiert. Aufbauend auf eine Einführung in die moderne beobachtende und theoretische Kosmologie wird die Entstehung von Strukturen und astronomischen Objekten im frühen Universum besprochen.
This introductory textbook has been designed by a team of experts for elementary university courses in astronomy and astrophysics. It starts with a detailed discussion of the structure and history of our own Galaxy, the Milky Way, and goes on to give a general introduction to normal and active galaxies including models for their formation and evolution. The second part of the book provides an overview of the wide range of cosmological models and discusses the Big Bang and the expansion of the Universe. Written in an accessible style that avoids complex mathematics, and illustrated in colour throughout, this book is suitable for self-study and will appeal to amateur astronomers as well as undergraduate students. It contains numerous helpful learning features such as boxed summaries, student exercises with full solutions, and a glossary of terms. The book is also supported by a website hosting further teaching materials.
This is a truly astonishing book, invaluable for anyone with an interest in astronomy. Physics Bulletin Just the thing for a first year university science course. Nature This is a beautiful book in both concept and execution. Sky & Telescope
In diesem kompetent geschriebenen Lehrbuch wird, ausgehend von der Beschreibung unserer Milchstraße, die Astronomie der Galaxien und ihrer großräumigen Verteilung eingehend dargestellt und schließlich im kosmologischen Kontext diskutiert. Aufbauend auf eine Einführung in die moderne beobachtende und theoretische Kosmologie wird die Entstehung von Strukturen und astronomischen Objekten im frühen Universum besprochen.
Dank sich stets verbessernder boden- und weltraumgestützter Teleskope stehen der Kosmologie inzwischen Daten zur Verfügung, die Rückschlüsse auf immer frühere Phasen des Universums und Vergleiche mit Modellvorstellungen erlauben. Daher gewinnt die Kosmologie in den Astronomiekursen der Universitäten beständig an Wichtigkeit. Die "Einführung in die Moderne Kosmologie" ist eine anschauliche und leicht verständliche Darstellung moderner kosmologischer Konzepte, die neben zahlreichen Beispielen und Übungsaufgaben auch Hinweise und Endergebnisse enthält, sodass das Erlernte sofort ausprobiert und kontrolliert werden kann. Das Buch ist klar eingeteilt und behandelt in sechs separaten Kapiteln Themen für Fortgeschrittene, darunter relativistische Kosmologie und Neutrino-Kosmologie. Die vorliegende Übersetzung der zweiten Auflage wurde wesentlich ergänzt und erweitert und umfasst neueste Beobachtungsergebnisse sowie zusätzliches Material zur empirischen Kosmologie und Strukturbildung.
Die Natur der Dunklen Materie gehört zu den spannendsten Fragen der Kosmologie. Die Bestseller-Autorin und Harvard-Professorin Lisa Randall nimmt uns in ihrem neuen Buch ›Dunkle Materie und Dinosaurier. Die erstaunlichen Zusammenhänge des Universums‹ mit auf eine Reise in die Welt der Physik und hilft uns zu verstehen, welche Rolle die Dunkle Materie bei der Entstehung unserer Galaxie, unseres Sonnensystems und sogar des Lebens selbst gespielt hat. Eindrucksvoll zeigt sie, wie die Wissenschaft neue Konzepte und Erklärungen für dieses weithin unbekannte Phänomen entwickelt und verwebt geschickt die Geschichte des Kosmos mit unserer eigenen. Ein Buch, das ein völlig neues Licht auf die tiefen Verbindungen wirft, die unsere Welt so maßgeblich mitgeprägt haben, und uns die außerordentliche Schönheit zeigt, die selbst den alltäglichsten Dingen innewohnt.
This book outlines the fundamentals of this fascinating branch of astronomy, and explores the forefront of astronomical research. The author’s passion for the topic shines with an intensity that rivals the book’s many colourful illustrations, and will deeply inspire the reader. The cogently written text introduces the reader to the astronomy of galaxies, their structure, their active galactic nuclei, their evolution and their large scale distribution. Starting with a detailed description of our Milky Way, and a review of modern observational and theoretical cosmology, the book goes on to examine the formation of structures and astronomical objects in the early universe.
This book provides a comprehensive, self-contained introduction to one of the most exciting frontiers in astrophysics today: the quest to understand how the oldest and most distant galaxies in our universe first formed. Until now, most research on this question has been theoretical, but the next few years will bring about a new generation of large telescopes that promise to supply a flood of data about the infant universe during its first billion years after the big bang. This book bridges the gap between theory and observation. It is an invaluable reference for students and researchers on early galaxies. The First Galaxies in the Universe starts from basic physical principles before moving on to more advanced material. Topics include the gravitational growth of structure, the intergalactic medium, the formation and evolution of the first stars and black holes, feedback and galaxy evolution, reionization, 21-cm cosmology, and more. Provides a comprehensive introduction to this exciting frontier in astrophysics Begins from first principles Covers advanced topics such as the first stars and 21-cm cosmology Prepares students for research using the next generation of large telescopes Discusses many open questions to be explored in the coming decade
Illustrations, photographs, star charts, moon maps, and scientific diagrams are compiled in a reference tool that explores the new solar system, the birth and death of stars, black holes, and space engineering.
Delineating the huge strides taken in cosmology in the past ten years, this much-anticipated second edition of Malcolm Longair's highly appreciated textbook has been extensively and thoroughly updated. It tells the story of modern astrophysical cosmology from the perspective of one of its most important and fundamental problems – how did the galaxies come about? Longair uses this approach to introduce the whole of what may be called "classical cosmology". What’s more, he describes how the study of the origin of galaxies and larger-scale structures in the Universe has provided us with direct information about the physics of the very early Universe.
The first comprehensive graduate-level textbook on one of the most dynamic areas of contemporary astronomy - the study of 'active galactic nuclei'.
Ideal for allied health and pre-nursing students, Alcamos Fundamentals of Microbiology, Body Systems Edition, retains the engaging, student-friendly style and active learning approach for which award-winning author and educator Jeffrey Pommerville is known. It presents diseases, complete with new content on recent discoveries, in a manner that is directly applicable to students and organized by body system. A captivating art program, learning design format, and numerous case studies draw students into the text and make them eager to learn more about the fascinating world of microbiology.
Galaxies are the building blocks of the Universe: standing like islands in space, they are where the stars are born and where extraordinary phenomena can be observed. Many exciting discoveries have been made: how a supermassive black hole lurks at the centre of every galaxy, how enormous forces are released when galaxies collide, and what the formation of young galaxies can tell us about the mysteries of Cold Dark Matter. In this Very Short Introduction, renowned science writer John Gribbin describes the extraordinary things that astronomers are learning about galaxies, and explains how this can shed light on the origins and structure of the Universe.
For every galaxy in the field or in clusters, there are about three galaxies in groups. The Milky Way itself resides in a group. Groups in the local universe offer the chance to study galaxies in environments characterized by strong interactions. In the cosmological context, groups trace large-scale structures better than clusters; the evolution of groups and clusters appears to be related. All these aspects of research are summarized in this book.
Es ist groß, dunkel und im wahrsten Sinne des Wortes maßlos: das Universum. Geht es um das Universum und seinen Ursprung, geraten Naturwissenschaften und Philosophie schnell an ihre Grenzen. Trotzdem oder vielleicht auch gerade deshalb gibt es hier viel Spannendes zu berichten. Wie entstehen Sterne, Planeten und Galaxien, wie wirken die Naturkräfte, was ist dunkle Materie, existiert das Universum ewig? Das sind nur einige der Fragen, auf die Sie in diesem Buch eine verständliche Antwort bekommen.
An Introduction to Modern Cosmology Third Edition is anaccessible account of modern cosmological ideas. The Big BangCosmology is explored, looking at its observational successes inexplaining the expansion of the Universe, the existence andproperties of the cosmic microwave background, and the origin oflight elements in the universe. Properties of the very earlyUniverse are also covered, including the motivation for a rapidperiod of expansion known as cosmological inflation. The thirdedition brings this established undergraduate textbook up-to-datewith the rapidly evolving observational situation. This fully revised edition of a bestseller takes an approachwhich is grounded in physics with a logical flow of chaptersleading the reader from basic ideas of the expansion described bythe Friedman equations to some of the more advanced ideas about theearly universe. It also incorporates up-to-date results from thePlanck mission, which imaged the anisotropies of the CosmicMicrowave Background radiation over the whole sky. The AdvancedTopic sections present subjects with more detailed mathematicalapproaches to give greater depth to discussions. Student problemswith hints for solving them and numerical answers are embedded inthe chapters to facilitate the reader’s understanding andlearning. Cosmology is now part of the core in many degree programs. Thiscurrent, clear and concise introductory text is relevant to a widerange of astronomy programs worldwide and is essential reading forundergraduates and Masters students, as well as anyone startingresearch in cosmology. Supplementary material, includingfull-colour images, updates and links for students and instructors,is available on the author’s website: ahref=""
A thorough introduction to modern ideas on cosmology and on the physical basis of the general theory of relativity, An Introduction to the Science of Cosmology explores various theories and ideas in big bang cosmology, providing insight into current problems. Assuming no previous knowledge of astronomy or cosmology, this book takes you beyond introductory texts to the point where you are able to read and appreciate the scientific literature, which is broadly referenced in the book. The authors present the standard big bang theory of the universe and provide an introduction to current inflationary cosmology, emphasizing the underlying physics without excessive technical detail. The book treats cosmological models without reliance on prior knowledge of general relativity, the necessary physics being introduced in the text as required. It also covers recent observational evidence pointing to an accelerating expansion of the universe. The first several chapters provide an introduction to the topics discussed later in the book. The next few chapters introduce relativistic cosmology and the classic observational tests. One chapter gives the main results of the hot big bang theory. Next, the book presents the inflationary model and discusses the problem of the origin of structure and the correspondingly more detailed tests of relativistic models. Finally, the book considers some general issues raised by expansion and isotropy. A reference section completes the work by listing essential formulae, symbols, and physical constants. Beyond the level of many elementary books on cosmology, An Introduction to the Science of Cosmology encompasses numerous recent developments and ideas in the area. It provides more detailed coverage than many other titles available, and the inclusion of problems at the end of each chapter aids in self study and makes the book suitable for taught courses.

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